COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 5721 THE 78TH NAME-LIST OF VARIABLE STARS

Size: px
Start display at page:

Download "COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 5721 THE 78TH NAME-LIST OF VARIABLE STARS"

Transcription

1 COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 5721 Konkoly Observatory Budapest 8 August 2006 HU ISSN THE 78TH NAME-LIST OF VARIABLE STARS KAZAROVETS, E.V. 1 ; SAMUS, N.N. 1,2 ; DURLEVICH, O.V. 2 ; KIREEVA, N.N. 1 ; PASTUKHOVA, E.N. 1 1 Institute of Astronomy, Russian Academy of Sciences, 48, Pyatnitskaya Str., Moscow , Russia [elena k@sai.msu.ru, kireeva@sai.msu.ru, pastukhova@sai.msu.ru, samus@sai.msu.ru] 2 Sternberg Astronomical Institute, University of Moscow, 13, University Ave., Moscow , Russia [gcvs@sai.msu.ru] The present 78th Name-List of Variable Stars contains all data necessary for identifications of 1706 new variables finally designated in The total number of named variable stars, not counting designated non-existing stars or stars subsequently identified with earlier-named variables, has now reached We are currently working on merging the electronic tables of the GCVS and the Name- Lists. Because of this, we decided to somewhat change the presentation of the 78th Name- List compared to the standard form of several previous lists, which followed the manner first introduced in the 67th Name-List (IBVS No. 2681, 1985). Thus, the main part of the 78th Name-List contains a single printed table, appended with two tables presented in the electronic form only. The printed Table 1, similar to Table 1 in the previous Name-Lists, contains the list of new variables arranged in the order of their right ascensions (2000.0). For each star, the table gives: its ordinal number; its GCVS name (an asterisk after it means the presence of a remark in the electronic Table E4, see below); the equatorial coordinates for the equinox (right ascensions to 0 ṣ 1 and declinations to 1 ); the range of variability (magnitudes in maximum and minimum light; sometimes the column Min gives, in parentheses, the amplitude of light variation; the symbol < means that the star, in minimum light, becomes fainter than the magnitude indicated; the system of magnitudes used. Here p are photographic magnitudes; r are instrumental red magnitudes; the symbols Rc, Ic designate magnitudes in Cousins RI system; Hp stands for magnitudes in the system of the Hipparcos Catalogue; * corresponds to unfiltered CCD magnitudes; the rest of designations are standard Johnson UBV RIJKL magnitudes or their more or less successful equivalents. In a small number of cases, the value of the variability amplitude (column Min, in parentheses) could not be expressed in the same system of magnitudes as the star s brightness; in such cases we indicate the photometric band for the amplitude separately. Then follows the type of variability according to the classification system described in the forewords to the first three volumes of the 4th GCVS edition (with the additions introduced in the 68th Name-List, IBVS No. 3058, 1987, in the 69th Name-List, IBVS No. 3323, 1989, in the 72nd Name-List, IBVS No. 4140, 1995, in the 75th Name-List, IBVS No. 4870, 2000, in the 76th Name-List, IBVS No. 5135, 2001; see also the description of variability types and distribution of stars over variability

2 2 IBVS 5721 types at In variance with the earlier Name-Lists, the last columns contain up to three references to the literature. The first reference is to the star s study that permitted us to include it into the Name-List, the second one indicates the paper containing a finding chart or refers to the Durchmusterung DM (BD, CoD, or CPD), or the Hubble Space Telescope Guide Star Catalog GSC, g2.2, or the USNO A1.0/A2.0/B1.0 catalog USNO, or the 2MASS catalog 2MASS, if the star can be found using one of them; in some cases, we add the third reference if information significant for the Name-List (mainly included in the electronic Table E3, see below) comes from a source different from that indicated in the first reference. The order of stars in Table 1 corresponds to the order of their right ascensions. Note that several stars named between Name-Lists No. 77 and No. 78 upon request from the IAU Bureau of Astronomical Telegrams have GCVS names, within their constellation, are not in their proper order by right ascension. The coordinates presented in the Name- List were taken from positional catalogues or found in the literature. Then, a short Table 2 follows. This is a list of variable stars earlier named not in their proper constellations, because of erroneous coordinates or of changes in the constellation boundaries (cf. N. N. Samus et al., 2006, Astronomy Letters, 32, 263, section The Variables to be Renamed ). The present Name-List contains new names for these variables. Their old names will not be given to any other variable, to avoid confusion. The electronic supplement to this paper contains two additional tables of the Name- List. Table E3 presents a preliminary catalogue of the newly-named variable stars. Its columns contain, besides the information described above for Table 1, also the following data: epoch (minimum for eclipsing variables and RV-type stars or maximum for all other stars, in Julian days minus ); variability period (in days); light curve asymmetry (M m) for pulsating variables or duration of minimum for eclipsing stars, in hundredths of the period; spectral type. The electronic Table E4 contains the list of variables arranged in the order of their variable star names within constellations. It can have several lines per variable. After the designation of a variable, its ordinal number from Table 1 is given, and then each line contains an identification with one of several major catalogues or an identification necessary to find this star in the papers referred to in Tables 1, E3 or in the papers with the first (or independent) announcement of the discovery of its variability. Some minimal remarks are given if necessary, also occupying a line, with * Rem in the beginning of the remark. The abbreviated names of the catalogues in Table E4 generally follow conventions of the GCVS or of the SIMBAD data base. We take the opportunity to announce corrections of several errors and misprints in earlier Name-Lists of Variable Stars, not announced earlier as lists of corrections in electronic issues of the IBVS. NL No. IBVS No. Position Printed Should be Table 2 V1191 Cyg V1991 Cyg Table 1, IL Cam Table 2, δ Sco Tables 1, 2 V1209 Tau = V738 Tau As usual, those wishing to find new and corrected GCVS and NSV catalogue information are asked to regularly visit our web site:

3 IBVS At our web site, there exists access to a table containing accurate coordinates and, whenever available, proper motions for GCVS stars (including Name-Lists) and for many NSV catalogue stars, taken from positional catalogues (referred to in the table) or measured by the GCVS team. The table is being continuously expanded in the course of our positional work. The positional information is based upon our new identifications, primarily using the best finding charts available, and checked via comparison with identifications by other authors whenever possible. We would like to thank many astronomers who sent us unpublished data, immediately responded to our requests to provide missing data or to correct erroneous data necessary for this Name-List. Also, thanks are due for sending us corrections to our catalogues and Name-Lists. This study was supported in part by Russian Foundation for Basic Research through grant , by the Programme Origin and Evolution of Stars and Galaxies of the Presidium of Russian Academy of Sciences, and by the Support Programme for Leading Scientific Schools of Russia. Our research has made extensive use of the excellent ASAS-3 data base.

4 4 IBVS 5721 Table V956 Cas B IS: CD Scl V RRAB V439 And ( 0.04 ) V BY 005 DM V957 Cas * SR: 006 USNO V958 Cas * SR: 006 GSC V959 Cas * EW 006 GSC EK Psc ( 0.02 ) B RPHS V960 Cas * SR 006 USNO V961 Cas* ( 0.40 ) V EB 010 GSC V440 And* * EA 006 GSC CE Scl* V EA 011 DM CF Scl V RS: 012 DM CP Phe V SRA V962 Cas* * EA CQ Phe V RRAB V963 Cas * SR: 006 USNO EU Cet ( 1.00 ) V RRAB 015 USNO EL Psc ( 0.22 ) V SRS 016 DM V964 Cas * SR: 006 USNO CR Phe V SRB 130 DM CG Scl V EA 011 DM V965 Cas * SR: 006 2MASS V441 And * EW 006 GSC CH Scl V EA: 011 DM EV Cet* ( 0.48 ) V EW 017 GSC V966 Cas ( 0.02 ) V BY 018 DM V442 And V BE 019 DM CS Phe V RRAB V443 And ( 0.02 ) V BY 018 DM V967 Cas * SRA 006 USNO V444 And * EW 006 GSC EW Cet ( 0.03 ) V BY 018 DM V445 And ( 0.03 ) V BY 018 DM V968 Cas * SR 006 USNO EM Psc* ( 0.45 ) V EW 010 GSC EG Tuc V SRS 130 DM EN Psc ( 0.02 ) V BY 018 DM V446 And* ( 0.09 ) V * 018 DM CT Phe V EA EO Psc ( 0.02 ) V RS 018 DM AR Tri V DSCTC: 022 GSC EX Cet ( 0.02 ) V BY 018 DM alpha Eri Hp BE 023 DM CU Phe ( 0.06 ) V GDOR: 024 DM EY Cet ( 0.03 ) V BY 018 DM V969 Cas ( 0.21 I ) V EA/RS V970 Cas * LB: 006 2MASS V971 Cas* ( 0.77 I ) V EA/RS: V972 Cas ( 0.39 Ic) Rc BE 026 DM V973 Cas ( 0.09 Ic) Rc BE 026 GSC V974 Cas ( 0.10 Ic) Rc BE 026 GSC V975 Cas ( 0.10 Ic) Rc BE 026 GSC V976 Cas ( 0.20 Ic) Rc BE 026 GSC V977 Cas ( 0.20 Ic) Rc BE 026 DM

5 IBVS V978 Cas ( 0.25 Ic) Rc BE 026 DM V979 Cas ( 0.10 Ic) Rc BE 026 GSC V980 Cas ( 0.15 Ic) Rc BE 026 GSC V981 Cas ( 0.15 Ic) Rc BE 026 DM V982 Cas ( 0.12 Ic) Rc BE 026 GSC V983 Cas ( 0.35 Ic) Rc BE 026 GSC V984 Cas ( 0.42 Ic) Rc BE 026 GSC V985 Cas ( 0.36 Ic) Rc BE 026 DM V986 Cas ( 0.05 Ic) Rc BE 026 GSC V987 Cas ( 0.05 ) V BY 005 DM EZ Cet ( 0.05 ) V BY 005 DM FF Cet ( 0.93 ) V RRAB 015 USNO FG Cet ( 0.82 ) V RRAB 015 USNO FH Cet* V EA 028 GSC FI Cet R UG: FK Cet ( 0.57 ) V RRAB 015 USNO FL Cet* ( 5.9 ) V E+XM 030 USNO V447 And ( 0.03 ) V RS 031 GSC AR For V SRA V988 Cas ( 0.02 ) B ACVO 032 DM FM Cet ( 0.98 ) V RRAB 015 USNO V448 And V M 332 GSC AS Tri ( 0.09 ) V DSCTC 033 DM FN Cet ( 0.04 ) V BY 018 DM FO Cet V GDOR 034 DM FP Cet ( 1.19 ) V RRAB 015 USNO V678 Per ( 0.02 ) B DSCTC: 035 DM V449 And * EW 332 GSC AZ Ari ( 0.02 ) V BY 018 DM FQ Cet ( 0.1 ) V EA 036 DM CV Phe ( 0.02 b ) V DSCTC 037 DM V450 And ( 0.02 ) V BY 018 DM V451 And ( 0.03 ) V BY 018 DM V989 Cas ( 0.03 ) V BY 018 DM V990 Cas* ( 0.02 ) V * 018 DM FR Cet* V * 038 DM CW Hyi V XM FS Cet ( 0.01 ) V R FT Cet ( 0.04 ) V BY 018 DM V679 Per * SR: 006 2MASS V680 Per* * EW 042 GSC BB Ari <17. * UGSU AS For <11.2 V M 332 USNO BC Ari ( 0.02 ) V BY 018 DM AT For V EA 011 DM IP Eri ( 0.04 ) V BY: 018 DM IQ Eri ( 0.5 ) V NL FU Cet* ( 0.05 ) V * 018 DM V681 Per * SR: 006 2MASS IR Eri ( 0.02 ) V RS 018 DM CX Hyi V SRS 130 DM V682 Per * M: 006 2MASS CY Hyi* V EW 130 DM IS Eri ( 0.06 ) V BY 018 DM

6 6 IBVS V683 Per ( 0.02 ) V BY 018 DM V684 Per * SR: 006 2MASS V991 Cas * M 006 2MASS V685 Per <15.0 * SR: 006 GSC V686 Per ( 0.04 ) V BY 018 DM V687 Per ( 0.02 ) V BY 018 DM LX Cam <14.5 * M: 006 2MASS V688 Per V BY 044 GSC V1220 Tau V EB 045 GSC V1221 Tau V BY 046 DM V1222 Tau * EW 047 GSC V1223 Tau * EW 047 GSC V1224 Tau V INT 048 GSC V689 Per V BY 044 GSC LY Cam <12.4 * SRA: 006 2MASS V690 Per ( 0.05 ) V DSCTC: V691 Per ( 0.03 ) V DSCTC: V1225 Tau ( 0.08 ) V GDOR 050 DM IT Eri V SRB 130 DM V692 Per ( 0.15 ) Ic INT V693 Per ( 0.07 ) Ic INT V694 Per Ic INT V695 Per ( 0.65 ) Ic INT V696 Per ( 0.26 ) Ic INT V697 Per Ic INT V698 Per Ic INT V699 Per ( 0.14 ) Ic INT V700 Per ( 0.18 ) Ic BY V701 Per ( 0.18 ) Ic BY V702 Per Ic INT V703 Per ( 0.06 ) Ic INT V704 Per ( 0.24 ) Ic INT V705 Per ( 0.04 ) V DSCTC: V706 Per ( 0.08 ) Ic INT V707 Per ( 0.24 ) Ic INT V708 Per ( 0.18 ) Ic INT V709 Per ( 0.08 ) Ic INT V710 Per Ic INT V711 Per ( 0.35 ) Ic INT 051 2MASS V712 Per Ic INT V713 Per Ic INT V714 Per ( 0.20 ) Ic INT 318 2MASS V715 Per ( 0.17 ) Ic INT V716 Per ( 0.29 ) Ic INT V717 Per ( 0.12 ) Ic INT V718 Per Ic E: V719 Per Ic INT V1226 Tau* ( 0.01: ) Ic * 007 2MASS V1227 Tau ( 0.15 ) V BY V720 Per * SR: 006 GSC V1228 Tau ( 0.02 v ) V DSCTC 057 DM V1229 Tau* V EA 058 DM LZ Cam* V EB MM Cam* ( 0.04 ) V * 018 DM

7 IBVS V1230 Tau* * EW 060 GSC MN Cam * DCEP 061 GSC MO Cam V BE 062 GSC V721 Per * SRA 332 2MASS MP Cam* * EB: MQ Cam * DCEP 061 GSC MR Cam * M 040 GSC IU Eri Hp DSCTC 024 DM V1231 Tau * RRC 063 USNO V722 Per ( 0.15 ) R BY V1232 Tau ( 0.05 ) V RS 018 DM IV Eri V RRAB 130 DM V1233 Tau ( 0.02 ) V BY 018 DM IW Eri V XM V1234 Tau* * EW 065 GSC V1235 Tau V DSCTC 022 GSC MS Cam ( 0.03 ) V BY 018 DM MT Cam* * EW IX Eri V BY 005 DM V536 Aur ( 0.03 ) V BY 018 DM V1648 Ori <14.6 V M 332 GSC V537 Aur ( 0.05 ) V DSCTC 067 GSC V1236 Tau ( 0.17 * ) V EA AS Col V RS: 046 DM V1649 Ori ( 0.01 b ) V DSCTC 037 DM V1237 Tau* ( 0.20 * ) V EW AF Lep V RS 071 DM V1650 Ori* : V INB: 038 DM AG Lep V BY 046 DM V1651 Ori ( 0.07 ) Ic INB 072 GSC V1652 Ori ( 0.07 ) Ic INB 072 USNO V1653 Ori ( 0.04 ) Ic INB 072 USNO V1654 Ori ( 0.05 ) Ic INB 072 USNO V1655 Ori ( 0.05 ) Ic INB 072 GSC V1656 Ori ( 0.15 ) Ic INB 072 USNO V1657 Ori ( 0.10 ) Ic INB 072 GSC V1658 Ori ( 0.32 ) Ic INB 072 USNO V1659 Ori ( 0.13 ) Ic INB 072 USNO V1660 Ori ( 0.08 ) Ic INB 072 USNO V1661 Ori ( 0.08 ) Ic INB 072 USNO V1662 Ori ( 0.10 ) Ic INB 072 USNO V1663 Ori ( 0.07 ) Ic INB 072 USNO V1664 Ori ( 0.17 ) Ic INB 072 USNO V1665 Ori ( 0.08 ) Ic INB 072 USNO V1666 Ori ( 0.11 ) Ic INB 072 USNO V1667 Ori ( 0.11 ) Ic INB 072 USNO V1668 Ori ( 0.08 ) Ic INB 072 USNO V1669 Ori ( 0.08 ) Ic INB 072 USNO AH Lep V BY 046 DM V1670 Ori ( 0.06 ) Ic INB 072 USNO V1671 Ori ( 0.10 ) Ic INB 072 2MASS V1672 Ori ( 0.06 ) Ic INB 072 USNO V1673 Ori ( 0.08 ) Ic INB 072 USNO V1674 Ori ( 0.10 ) Ic INB 072 2MASS

8 8 IBVS V1675 Ori ( 0.08 ) Ic INB 072 USNO V1676 Ori ( 0.16 Ic) J INB 072 USNO V1677 Ori ( 0.10 ) Ic INB 072 USNO V1678 Ori ( 0.09 ) Ic INB 072 USNO V1679 Ori ( 0.14 ) Ic INB 072 USNO V1680 Ori ( 0.30 ) Ic INB 072 USNO V1681 Ori ( 0.10 ) Ic INB 072 2MASS V1682 Ori ( 0.07 ) Ic INB 072 USNO V1683 Ori ( 0.10 ) Ic INB 072 2MASS V1684 Ori ( 0.10 ) Ic INB 072 2MASS V1685 Ori ( 0.14 ) Ic INB 072 USNO V1686 Ori ( 0.04 ) Ic INB 072 GSC V1687 Ori ( 0.11 ) Ic INB 072 2MASS V1688 Ori ( 0.10 ) Ic INB 072 USNO V1689 Ori ( 0.09 ) Ic INB 072 USNO V1690 Ori ( 0.04 ) Ic INB 072 USNO V1691 Ori ( 0.09 ) Ic INB 072 2MASS V1692 Ori ( 0.08 ) Ic INB 072 USNO V1693 Ori ( 0.20 ) Ic INB 072 USNO V1694 Ori ( 0.44 ) Ic INB 072 USNO V1695 Ori ( 0.16 ) Ic INB 072 2MASS V1696 Ori ( 0.22 ) Ic INB 072 USNO V1697 Ori ( 0.08 ) Ic INB 072 2MASS V1698 Ori ( 0.10 ) Ic INB 072 2MASS V1699 Ori ( 0.31 ) Ic INB 072 2MASS V1700 Ori ( 0.07 ) Ic INB 072 USNO V1701 Ori ( 0.11 ) Ic INB 072 GSC V1702 Ori ( 0.05 ) Ic INB 072 USNO V1703 Ori ( 0.09 ) Ic INB 072 USNO V1704 Ori ( 0.22 ) Ic INB 072 2MASS V1705 Ori ( 0.11 ) Ic INB 072 USNO V1706 Ori ( 0.06 ) Ic INB 072 USNO V1707 Ori ( 0.10 ) Ic INB 072 2MASS V1708 Ori ( 0.07 ) Ic INB 072 USNO V1709 Ori ( 0.18 ) Ic INB 072 USNO V1710 Ori ( 0.05 ) Ic INB 072 2MASS V1711 Ori ( 0.05 ) Ic INB 072 USNO V1712 Ori ( 0.6 ) Ic INB 072 2MASS V1713 Ori ( 0.09 ) Ic INB 072 2MASS V1714 Ori ( 0.16 ) Ic INB 072 2MASS V1715 Ori ( 0.05 ) Ic INB 072 2MASS V1716 Ori ( 0.15 ) Ic INB 072 USNO V1717 Ori ( 0.30 ) Ic INB 072 2MASS V1718 Ori ( 0.34 ) Ic INT 072 2MASS V1719 Ori ( 0.08 ) Ic INB 072 2MASS V1720 Ori ( 0.12 ) Ic INB 072 2MASS V1721 Ori ( 0.06 ) Ic INB 072 2MASS V1722 Ori ( 0.11 ) Ic INB 072 USNO V1723 Ori ( 0.18 ) Ic INB 072 USNO V1724 Ori ( 0.05 ) Ic INB 072 USNO V1725 Ori ( 0.10 ) Ic INB 072 2MASS V1726 Ori ( 0.08 ) Ic INB 072 2MASS V1727 Ori ( 0.11 ) Ic INB 072 2MASS V1728 Ori ( 0.11 ) Ic INB 072 USNO

9 IBVS V1729 Ori ( 0.29 ) Ic INB 072 USNO V1730 Ori ( 0.21 ) Ic INB 072 2MASS V1731 Ori ( 0.08 ) Ic INB 072 2MASS V1732 Ori ( 0.10 ) Ic INB 072 USNO V1733 Ori ( 0.16 ) Ic INB 072 USNO V1734 Ori ( 0.09 ) Ic INB 072 2MASS V1735 Ori ( 0.10 ) Ic INB 072 USNO V1736 Ori ( 0.10 ) Ic INB 072 2MASS V1737 Ori ( 0.11 ) Ic INB 072 USNO V1738 Ori ( 0.04 ) Ic INB 072 USNO V1739 Ori ( 0.06 ) Ic INB 072 USNO V1740 Ori ( 0.07 ) Ic INB 072 USNO V1741 Ori ( 0.13 ) Ic INB 072 2MASS V1742 Ori ( 0.10 ) Ic INB 072 USNO V1743 Ori ( 0.21 ) Ic INB 072 2MASS V1744 Ori ( 0.06 ) Ic INB 072 2MASS V1745 Ori ( 0.11 ) Ic INB 072 2MASS V1746 Ori ( 0.10 ) Ic INB 072 2MASS V1747 Ori ( 0.07 ) Ic INB 072 USNO V1748 Ori ( 0.16 ) Ic INB 072 USNO V1749 Ori ( 0.07 ) Ic INB 072 USNO V1750 Ori ( 0.13 ) Ic INB 072 2MASS V1751 Ori ( 0.10 ) Ic INB 072 2MASS V1752 Ori ( 0.04 ) Ic INB 072 USNO V1753 Ori ( 0.06 ) Ic INB 072 2MASS V1754 Ori ( 0.11 ) Ic INB 072 USNO V1755 Ori ( 0.12 ) Ic INB 072 2MASS V1756 Ori ( 0.18 ) Ic INB 072 USNO V1757 Ori ( 0.24 ) Ic INB 072 2MASS V1758 Ori ( 0.05 ) Ic INB 072 USNO V1759 Ori ( 0.08 ) Ic INB 072 2MASS V1760 Ori ( 0.41 ) Ic INB 072 GSC V1761 Ori ( 0.11 ) Ic INB 072 2MASS V1762 Ori ( 0.15 ) Ic INB 072 USNO V1763 Ori ( 0.23 ) Ic INB 072 USNO V1764 Ori ( 0.15 ) Ic INB 072 USNO V1765 Ori ( 0.05 ) Ic INB 072 GSC V1766 Ori ( 0.05: ) Ic INB 072 USNO V1767 Ori ( 0.15 ) Ic INB 072 2MASS V1768 Ori ( 0.22 ) Ic INB 072 USNO V1769 Ori ( 0.05 ) Ic INB 072 USNO V1770 Ori ( 0.15 ) Ic INB 072 2MASS V1771 Ori ( 0.23 ) Ic INB 072 USNO V1772 Ori ( 0.09 ) Ic INB 072 GSC V1773 Ori ( 0.05 ) Ic INB 072 USNO V1774 Ori ( 0.13 ) Ic INB 072 USNO V1775 Ori ( 0.07 ) Ic INB 072 USNO V1776 Ori ( 0.25 ) Ic INB 072 USNO V1777 Ori ( 0.06 ) Ic INB 072 GSC AT Col V BY 046 DM V1778 Ori ( 0.21 ) Ic INB 072 USNO V1779 Ori ( 0.09 ) Ic INB 072 USNO V1780 Ori ( 0.12 ) Ic INB 072 USNO V1781 Ori ( 0.08 ) Ic INB 072 USNO

10 10 IBVS V1782 Ori ( 0.15 ) Ic INB 072 USNO V1783 Ori ( 0.09 ) Ic INB 072 USNO V1784 Ori ( 0.16 ) Ic INB 072 USNO V1785 Ori ( 0.10 ) Ic INB 072 USNO V1786 Ori ( 0.04 ) Ic INB 072 USNO V1787 Ori V INA 038 GSC V1788 Ori V INA 038 DM V1789 Ori ( 0.11 ) Ic INB 072 GSC AI Lep ( 0.05 ) V RS 018 DM V1790 Ori ( 0.01 b ) V DSCTC 037 DM V1791 Ori V INB: 038 USNO V1792 Ori V INB 038 GSC V538 Aur Hp BY 005 DM V1238 Tau* V EW 130 DM AK Lep ( 0.06 ) V BY 074 DM V1647 Ori* <20. V FU BC Dor V UG V1239 Tau* V EA: 130 GSC V539 Aur ( 0.55 Rc) V DSCT V540 Aur ( 0.23 Rc) V EA: V541 Aur ( 0.4 Rc) V EA: V542 Aur* ( 0.35 Rc) V EW V543 Aur* ( 0.68 Rc) V EW V544 Aur* ( 0.33 Rc) V EW V545 Aur ( 0.39 Rc) V RRC: V1793 Ori V INT 038 DM V546 Aur* V GDOR: V547 Aur* V GDOR: V548 Aur* V DSCT V549 Aur <16.40 V EA V550 Aur V DSCTC V551 Aur* V EA+DSCT V575 Pup* ( 0.04 ) V RS 046 DM AU Col ( 0.04 b ) V DSCTC 037 DM V371 Gem* V DCEP V352 CMa V BY 046 DM V552 Aur* p AM: V1794 Ori <18.2 B M V1795 Ori <19.8 B M V1796 Ori <20.0 B M V1797 Ori <19.8 B M V353 CMa ( 0.02 ) V BY 018 DM MU Cam* R XM V354 CMa V M 130 USNO V848 Mon ( 0.02 ) V BY 018 DM AI Pic <15.0 V M 130 USNO V355 CMa <14.3 V M AK Pic V BY 046 DM V849 Mon <14.8 V SRB 130 USNO V356 CMa ( 0.02 ) V BY: 018 DM V850 Mon ( 0.03 ) V BY 018 DM V553 Aur Hp GDOR 091 DM V576 Pup <15.5 V M 332 USNO V372 Gem* ( 0.50 ) V EB 092 GSC

11 IBVS V851 Mon* V ACV: V852 Mon* V EW: V853 Mon* V EW V854 Mon V GDOR V855 Mon V GDOR V856 Mon V ACV: V857 Mon* V EW V858 Mon* V EW: V859 Mon* V EB V577 Pup <14.4 V M 090 2MASS V860 Mon* V EA 130 DM V861 Mon* V EA 095 GSC V862 Mon ( 0.02 ) V BY 018 DM V863 Mon* V EB 130 DM DW Lyn ( 0.03 ) B RPHS 096 GSC V373 Gem* V EB 011 DM CX CMi* V EW 097 GSC V374 Gem <14. V M V864 Mon V EW 130 GSC CY CMi V SRD 099 DM CZ CMi V EW 097 GSC V578 Pup <14.5 V M 130 USNO V579 Pup* V EA 130 GSC V580 Pup V SRA 130 GSC V357 CMa V SRA 090 DM V358 CMa* ( 0.10 ) V WR: V359 CMa V SRA 130 GSC V865 Mon V SRB 095 GSC V375 Gem* V EB 319 GSC V575 Car* V EA 011 DM V581 Pup* V EW 011 DM V376 Gem ( 0.03 ) V BY 018 DM DX Lyn ( 0.02 ) V BY 018 DM V582 Pup* V EA 011 DM V866 Mon V EA 095 GSC V867 Mon ( 0.02 ) V BY 018 DM V868 Mon V EB 094 DM V869 Mon ( 0.02 ) V BY 018 DM V583 Pup V EB 011 DM V574 Pup : V NA V870 Mon <12. V M 103 GSC DD CMi Hp GDOR 091 DM V377 Gem ( 0.05 ) V BY 005 DM V584 Pup V SRB 130 DM V585 Pup <14.0 V M 130 USNO DY Lyn* V EA 104 DM V586 Pup V M 090 USNO V587 Pup* V EA 011 DM V871 Mon V EA 322 DM HM Cnc ( 1.08 ) I XM: V588 Pup* <14.5 V M 130 USNO DE CMi ( 0.06 ) B DSCTC 106 DM V589 Pup* V EA 011 DM DZ Lyn V EB: 104 DM

12 12 IBVS EE Lyn V DSCTC 022 DM V590 Pup V M HN Cnc* V EW 065 GSC V591 Pup <14.4 V M 332 USNO V576 Car* K * 108 2MASS V397 Hya ( 0.03 ) V BY 018 DM EF Lyn Hp GDOR 091 DM MV Cam * SRA 332 GSC EG Lyn R XM V577 Car V M 130 USNO V592 Pup V RS 046 DM V593 Pup <14.6 V M 088 USNO V594 Pup V RV 332 GSC V398 Hya V M 090 GSC V595 Pup V EA 040 GSC V399 Hya ( 0.02 ) V BY 018 DM LS UMa ( 0.20 ) V GDOR 091 DM XX Vol <14.8 V M 040 GSC V400 Hya <15.0 V M 332 USNO CR Pyx* V EB 130 DM CS Pyx ( 0.03 ) V BY 110 DM HO Cnc ( 0.03 ) V BY 018 DM CT Pyx ( 0.04 ) V BY 018 DM V401 Hya ( 0.05: ) V BY 005 DM ES Cha* ( 0.14 ) V INT V388 Vel V INA 038 2MASS ET Cha* ( 0.7 ) V INT V578 Car <14.0 V M 332 USNO CU Pyx* V EA 112 DM LT UMa ( 0.03 ) V BY 018 DM HP Cnc ( 0.02 ) V BY 018 DM HQ Cnc* ( 0.20 ) V E 113 USNO HR Cnc ( 0.12 ) V RS: 113 USNO HS Cnc ( 0.14 ) V EW 323 GSC HT Cnc* ( 0.06 ) V E: 115 GSC HU Cnc* V RS: 323 GSC HV Cnc ( 0.00 ) V EA 311 GSC HW Cnc* ( 0.07 ) V RS: 115 GSC HX Cnc* ( 0.08 ) V RS: 115 GSC HY Cnc ( 0.07 ) V RS: 115 GSC V402 Hya ( 0.12 ) V BY 046 DM HZ Cnc* ( 0.03 ) R * V389 Vel <12.5 V SRA 130 GSC II Cnc ( 0.05 ) V BY 018 DM V403 Hya V M 130 GSC IK Cnc ( 0.03 ) V BY 018 DM IL Cnc* * EW 060 GSC V390 Vel* V RV: 119 DM V391 Vel V INA 038 GSC DS Oct <14.8 V M IM Cnc* V EA 225 GSC V392 Vel V BE 038 DM CV Pyx V SRA 130 GSC V393 Vel V SRB 332 USNO

13 IBVS V394 Vel V SRB 130 GSC V395 Vel <14.0 V M 332 GSC XY Vol V M 130 USNO EH Lyn * EW 060 GSC CW Pyx <15.0 V M 332 GSC XZ Vol V SRA V579 Car V SRA 130 USNO YY Vol V SRA V404 Hya* * EW 122 GSC V405 Hya ( 0.03 ) V BY 018 DM V580 Car <14.7 V M 130 USNO V581 Car <14.4 V M 130 USNO V582 Car V SRA: V406 Hya V NL 123 USNO V396 Vel <13.8 V M 332 USNO CX Pyx V SRA 130 GSC CY Pyx* V E: 046 DM V407 Hya V SRB V583 Car V SRA 130 GSC V408 Hya V SRB 130 DM V409 Hya V EW V397 Vel V SRB 130 USNO V584 Car V M V410 Hya V EA 011 DM V585 Car <15.0 V M: 130 USNO V411 Hya V SRB 130 DM EI Lyn ( 0.03 ) V SXARI 127 DM V412 Hya* : V EA V413 Hya V SRB 130 GSC IN Cnc* * EB 060 GSC V586 Car V M IO Cnc* * EW 060 GSC IP Cnc ( 0.02 ) V BY 018 DM CZ Pyx* V SRB 130 GSC DD Pyx V SRB 130 DM V587 Car V SRB: IQ Cnc* * EW 122 GSC DE Pyx V RRC 130 GSC V588 Car <14.2 V M 332 USNO DF Pyx <14.3 V M 130 USNO V414 Hya V RS: 131 DM EU Cha <15.2 V M 332 USNO V589 Car <15.0 V M 040 USNO LU UMa* Hp GDOR 091 DM DG Pyx V SRA 130 GSC V415 Hya Hp GDOR: 091 DM V590 Car V RRAB V591 Car V LB DH Pyx V LB 130 DM WY LMi * RRAB 063 GSC GS Leo ( 0.06 ) V BY 018 DM LV UMa ( 0.03 ) V DSCTC: V592 Car* V EW V593 Car V M 130 GSC

14 14 IBVS V594 Car V EA V595 Car V M GT Leo ( 0.04 ) V BY 018 DM VZ Sex V XM 310 USNO GU Leo* * EW 135 GSC V596 Car V IA 038 DM WW Sex* V EA 322 DM BF Ant ( 0.01 ) V DSCTC 024 DM LW UMa V DSCTC 022 DM V416 Hya Hp GDOR 024 DM V417 Hya ( 0.03 ) V BY 018 DM WX Sex* V EW 017 GSC WY Sex* ( 0.36 ) V EW 017 GSC GV Leo* V EW 306 GSC WZ Sex* V EB 094 DM LX UMa ( 0.05 ) V BY 018 DM XX Sex V EW 094 DM V597 Car V SRB 130 GSC GW Leo * EW 060 GSC V398 Vel ( 0.03 ) V ELL: 136 DM XY Sex ( 0.08 ) V R V399 Vel ( 0.02 ) V BCEP: 136 DM XZ Sex <10.4 V SRA 103 GSC WZ LMi* * EW 135 GSC XX LMi* * EW 122 GSC XY LMi* * EW 122 GSC V418 Hya ( 0.02 ) V BY: 018 DM YY Sex V XM 137 USNO V598 Car* V EA 011 DM V419 Hya ( 0.02 ) V BY 018 DM LY UMa V NL 138 USNO LZ UMa ( 0.02 ) V BY 018 DM V400 Vel <14.8 V M 090 USNO V599 Car V IA 038 DM GX Leo B SRS 141 DM GY Leo ( 0.03 ) V BY 018 DM XZ LMi* ( 0.03 ) V RS: 018 DM GZ Leo V RS 141 DM AB Crt ( 0.03 ) V BY 018 DM YY LMi* ( 0.06 ) V RS: 018 DM HH Leo V BY 046 DM V600 Car V M MM UMa* ( 0.01 ) Ic * HI Leo* ( 0.8 ) V EB 017 GSC V601 Car V SRA 290 DM MN UMa Hp BY 005 DM MO UMa * RRC 144 GSC V602 Car V SRC 130 DM HK Leo* V R MP UMa * DSCT: 144 GSC MQ UMa * EW 144 GSC V1048 Cen* I CEP(B) 147 DM MR UMa V UGSU MS UMa* * EW 144 GSC 332

15 IBVS MT UMa* * EW 144 GSC MU UMa * RRC 144 GSC V1049 Cen V SRA V1050 Cen V M V1051 Cen V EA 011 DM MV UMa* ( 0.02 ) V RS 018 DM V1052 Cen V IA 038 DM MQ Mus <14.4 V M 090 USNO MR Mus* V EA 011 DM MW UMa ( 0.49 ) Rc EA HL Leo ( 0.06 ) V BY 018 DM MX UMa ( 0.08 ) B DSCTC 152 DM MS Mus V DCEP 130 DM PQ Vir ( 0.03 ) V BY: 018 DM MY UMa ( 0.03 ) V BY 018 DM PR Vir ( 0.05 ) V BY 018 DM PS Vir* V EW 154 GSC LV Com ( 0.03 ) V BY 018 DM DN CVn V RRC 155 GSC MZ UMa ( 0.02 ) V BY 018 DM DZ Cru <20. V N: PT Vir* * EW 135 GSC V420 Hya* V E: 100 DM NN UMa ( 0.03 ) V BY: 018 DM MW Cam Hp DSCT 157 DM V1053 Cen* V EW 011 DM NO UMa* ( 0.03 ) V RS: 005 DM V1054 Cen* V EW 011 DM DO CVn ( 0.02 ) V BY 018 DM DP CVn ( 0.07 ) V BY: 018 DM PU Vir* * EW 060 GSC DQ CVn* * EW 264 GSC NP UMa ( 0.03 ) V BY 018 DM DR CVn* * EW 264 GSC V1055 Cen <15.0 V M 090 USNO DS CVn V RRAB 264 GSC VZ Crv ( 0.03 ) V BY 018 DM LW Com ( 0.10 ) V BY 160 DM DT CVn ( 0.03 ) B DSCTC 037 DM LX Com ( 0.05 ) V BY 018 DM DU CVn* * EW 161 GSC EE Cru ( 0.05 ) B LPB: 162 GSC EF Cru ( 0.01 ) V BCEP 162 GSC EG Cru ( 0.01 ) V BCEP: 162 GSC EH Cru ( 0.01 ) B BCEP: 162 GSC DV CVn V RRC 155 GSC EI Cru ( 0.01 ) V BCEP 162 USNO LY Com V RRC 155 GSC PV Vir V DSCTC 022 GSC LZ Com V RRC 155 GSC V1056 Cen <11.5 V M 090 GSC MM Com* * EW 264 GSC MN Com* ( 0.05 ) Ic * 007 2MASS DW CVn ( 0.04 ) V BY: 018 DM

16 16 IBVS PW Vir <15.1 V M 090 GSC PX Vir ( 0.04 ) V BY 018 DM MO Com V RRAB 155 GSC V421 Hya* ( 0.02 ) Ic * DX CVn* * EW 264 GSC MP Com Hp GDOR 165 DM MT Mus V SRA 130 GSC MQ Com V RRAB 155 GSC PY Vir* V EW 094 DM DY CVn* * EW 264 GSC V1057 Cen* V EW V1058 Cen ( 0.2 * ) R IS MR Com* * EW 264 GSC DZ CVn V RRAB 155 GSC V1047 Cen <11.0 V N PZ Vir r AM NQ UMa ( 0.04 ) V BY 018 DM QQ Vir ( 0.05 ) B RPHS EV Cha V M EE CVn* * EW 264 GSC EF CVn* * EW 264 GSC GV Boo* * EW 264 GSC EG CVn * EW 264 GSC EH CVn* * EW 161 GSC V1059 Cen* <15.0 V M 090 GSC QR Vir V SRA 090 DM V1060 Cen <11.5 V SRA: 090 GSC QS Vir U EA+UV QT Vir ( 0.02 b ) V DSCTC 037 DM GW Boo V EW 104 DM MP Dra ( 0.03 ) V BY 018 DM GX Boo ( 0.24 V ) * EW: 161 GSC EI CVn* * EW 264 GSC QU Vir* * EW 135 GSC GY Boo ( 0.03 ) V BY 018 DM V1061 Cen* V EA 011 DM DF Cir ( 0.08 ) V RS 046 DM QV Vir * SXPHE 172 GSC GZ Boo ( 0.04 ) V BY 018 DM HH Boo* V EW 104 GSC HI Boo* ( 0.35 ) V R: 173 GSC HK Boo* ( 0.09 ) V RS 018 DM HL Boo ( 0.03 ) V EA: 018 DM HM Boo ( 0.02 ) V E:/RS 018 DM V1062 Cen <14.5 V M QW Vir * RRC 172 GSC KS Lib <13.9 V M 090 USNO HN Boo ( 0.04 ) V BY 018 DM QX Vir* V EW 130 GSC KT Lib ( 0.1 : ) V SXPHE 175 GSC KU Lib Hp BY 005 DM V1063 Cen ( 0.02 ) B DSCTC 176 DM KV Lib * SXPHE 063 GSC HO Boo ( 0.02 ) V BY 018 DM

Parts Manual. EPIC II Critical Care Bed REF 2031

Parts Manual. EPIC II Critical Care Bed REF 2031 EPIC II Critical Care Bed REF 2031 Parts Manual For parts or technical assistance call: USA: 1-800-327-0770 2013/05 B.0 2031-109-006 REV B www.stryker.com Table of Contents English Product Labels... 4

More information

A L A BA M A L A W R E V IE W

A L A BA M A L A W R E V IE W A L A BA M A L A W R E V IE W Volume 52 Fall 2000 Number 1 B E F O R E D I S A B I L I T Y C I V I L R I G HT S : C I V I L W A R P E N S I O N S A N D TH E P O L I T I C S O F D I S A B I L I T Y I N

More information

Studies of RV Tauri and SRD Variables

Studies of RV Tauri and SRD Variables 176 Studies of RV Tauri and SRD Variables Percy, JAAVSO Volume 43, 2015 John R. Percy Department of Astronomy and Astrophysics and Dunlap Institute for Astronomy and Astrophysics, University of Toronto,

More information

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 6xxx

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 6xxx COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 6xxx Konkoly Observatory Budapest x Xxxx 2012 HU ISSN 0374 0676 MINIMA OF ECLIPSING BINARIES AND NEW EPHEMERIDES FOR GSC 03881-00579

More information

176 5 t h Fl oo r. 337 P o ly me r Ma te ri al s

176 5 t h Fl oo r. 337 P o ly me r Ma te ri al s A g la di ou s F. L. 462 E l ec tr on ic D ev el op me nt A i ng er A.W.S. 371 C. A. M. A l ex an de r 236 A d mi ni st ra ti on R. H. (M rs ) A n dr ew s P. V. 326 O p ti ca l Tr an sm is si on A p ps

More information

Baltic Astronomy, vol. 24, , 2015 A STUDY OF DOUBLE- AND MULTI-MODE RR LYRAE VARIABLES. A. V. Khruslov 1,2

Baltic Astronomy, vol. 24, , 2015 A STUDY OF DOUBLE- AND MULTI-MODE RR LYRAE VARIABLES. A. V. Khruslov 1,2 Baltic Astronomy, vol. 24, 379 386, 2015 A STUDY OF DOUBLE- AND MULTI-MODE RR LYRAE VARIABLES A. V. Khruslov 1,2 1 Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya str. 48, Moscow 119017,

More information

OH BOY! Story. N a r r a t iv e a n d o bj e c t s th ea t e r Fo r a l l a g e s, fr o m th e a ge of 9

OH BOY! Story. N a r r a t iv e a n d o bj e c t s th ea t e r Fo r a l l a g e s, fr o m th e a ge of 9 OH BOY! O h Boy!, was or igin a lly cr eat ed in F r en ch an d was a m a jor s u cc ess on t h e Fr en ch st a ge f or young au di enc es. It h a s b een s een by ap pr ox i ma t ely 175,000 sp ect at

More information

CIRCULAR No JULY

CIRCULAR No JULY BRITISH ASTRONOMICAL ASSOCIATION: CIRCULAR No. 19 1974 JULY VARIABLE STAR SECTION Director: Charts: Secretary: J E Isles S J Anderson D R B Saw 292 Caledonian Road 20 Bloomfield Ave 12 Taylor Road London

More information

Visual Minima Timings of Eclipsing Binaries Observed in the Years

Visual Minima Timings of Eclipsing Binaries Observed in the Years Visual Minima Timings of Eclipsing Binaries Observed in the Years 1992-1996 PETR MOLÍK 1 1) Okružní 103/III, 392 01 Soběslav, Czech Republic; e-mail: Petr.Molik@vupp.cz Abstract: This paper contains a

More information

Period Analysis of AAVSO Visual Observations of 55 Semiregular (SR/SRa/SRb) Variable Stars

Period Analysis of AAVSO Visual Observations of 55 Semiregular (SR/SRa/SRb) Variable Stars Percy and Tan, JAAVSO Volume 41, 2013 1 Period Analysis of AAVSO Visual Observations of 55 Semiregular (SR/SRa/SRb) Variable Stars John R. Percy Paul Jx Tan Department of Astronomy and Astrophysics, University

More information

Applications and Remote Sensing, Penteli, Athens, Hellas; noa.gr. Astronomy and Mechanics, Zografos, Athens, Hellas; phys.uoa.

Applications and Remote Sensing, Penteli, Athens, Hellas; noa.gr. Astronomy and Mechanics, Zografos, Athens, Hellas; phys.uoa. Binaries with aδscuti component: Results from a long term observational survey, updated catalogue and future prospects arxiv:1506.07409v1 [astro-ph.sr] 24 Jun 2015 Alexios Liakos 1 and Panagiotis Niarchos

More information

T h e C S E T I P r o j e c t

T h e C S E T I P r o j e c t T h e P r o j e c t T H E P R O J E C T T A B L E O F C O N T E N T S A r t i c l e P a g e C o m p r e h e n s i v e A s s es s m e n t o f t h e U F O / E T I P h e n o m e n o n M a y 1 9 9 1 1 E T

More information

Trade Patterns, Production networks, and Trade and employment in the Asia-US region

Trade Patterns, Production networks, and Trade and employment in the Asia-US region Trade Patterns, Production networks, and Trade and employment in the Asia-U region atoshi Inomata Institute of Developing Economies ETRO Development of cross-national production linkages, 1985-2005 1985

More information

BAV-results of observations. Joachim Hübscher -address: BAV Mitteilungen No November 2014

BAV-results of observations. Joachim Hübscher  -address: BAV Mitteilungen No November 2014 BAV Mitteilungen BAV-results of observations Joachim Hübscher E-Mail-address: publicat@bav-astro.de BAV Mitteilungen No. 236 November 2014 Abstract: This 79th compilation contains especially the results

More information

P a g e 5 1 of R e p o r t P B 4 / 0 9

P a g e 5 1 of R e p o r t P B 4 / 0 9 P a g e 5 1 of R e p o r t P B 4 / 0 9 J A R T a l s o c o n c l u d e d t h a t a l t h o u g h t h e i n t e n t o f N e l s o n s r e h a b i l i t a t i o n p l a n i s t o e n h a n c e c o n n e

More information

Cataraqui Source Protection Area Stream Gauge Locations

Cataraqui Source Protection Area Stream Gauge Locations Cqu u P m Gu s Ts Ez K Ts u s sp E s ms P Ps s m m C Y u u I s Ts x C C u R 4 N p Ds Qu H Em us ms p G Cqu C, s Ks F I s s Gqu u Gqu s N D U ( I T Gqu C s C, 5 Rs p, Rs 15, 7 N m s m Gus - Ps P f P 1,

More information

Key parameters of W UMa-type contact binaries discovered by HIPPARCOS. S. O. Selam

Key parameters of W UMa-type contact binaries discovered by HIPPARCOS. S. O. Selam A&A 416, 1097 1105 (2004) DOI: 10.1051/0004-6361:20034578 c ESO 2004 Astronomy & Astrophysics Key parameters of W UMa-type contact binaries discovered by HIPPARCOS S. O. Selam Ankara University, Faculty

More information

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS. Reports on New Discoveries

COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS. Reports on New Discoveries 1 COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Konkoly Observatory Budapest HU ISSN 0374 0676 Reports on New Discoveries (This will appear as IBVS No. 6100.) Previous reports

More information

P a g e 3 6 of R e p o r t P B 4 / 0 9

P a g e 3 6 of R e p o r t P B 4 / 0 9 P a g e 3 6 of R e p o r t P B 4 / 0 9 p r o t e c t h um a n h e a l t h a n d p r o p e r t y fr om t h e d a n g e rs i n h e r e n t i n m i n i n g o p e r a t i o n s s u c h a s a q u a r r y. J

More information

IDENTIFICATION CHARTS FOR 42 VARIABLE STARS DISCOVERED AT HARVARD. Arville D. Walker and Margaret Olmsted Harvard College Observatory

IDENTIFICATION CHARTS FOR 42 VARIABLE STARS DISCOVERED AT HARVARD. Arville D. Walker and Margaret Olmsted Harvard College Observatory IDENTIFICATION CHARTS FOR 42 VARIABLE STARS DISCOVERED AT HARVARD Arville D. Walker and Margaret Olmsted Harvard College Observatory Some time ago Dr. G. H. Herbig, acting for Commissions 27 and 29 of

More information

35H MPa Hydraulic Cylinder 3.5 MPa Hydraulic Cylinder 35H-3

35H MPa Hydraulic Cylinder 3.5 MPa Hydraulic Cylinder 35H-3 - - - - ff ff - - - - - - B B BB f f f f f f f 6 96 f f f f f f f 6 f LF LZ f 6 MM f 9 P D RR DD M6 M6 M6 M. M. M. M. M. SL. E 6 6 9 ZB Z EE RC/ RC/ RC/ RC/ RC/ ZM 6 F FP 6 K KK M. M. M. M. M M M M f f

More information

Executive Committee and Officers ( )

Executive Committee and Officers ( ) Gifted and Talented International V o l u m e 2 4, N u m b e r 2, D e c e m b e r, 2 0 0 9. G i f t e d a n d T a l e n t e d I n t e r n a t i o n a2 l 4 ( 2), D e c e m b e r, 2 0 0 9. 1 T h e W o r

More information

THE TRANSLATION PLANES OF ORDER 49 AND THEIR AUTOMORPHISM GROUPS

THE TRANSLATION PLANES OF ORDER 49 AND THEIR AUTOMORPHISM GROUPS MATHEMATICS OF COMPUTATION Volume 67, Number 223, July 1998, Pages 1207 1224 S 0025-5718(98)00961-2 THE TRANSLATION PLANES OF ORDER 49 AND THEIR AUTOMORPHISM GROUPS C. CHARNES AND U. DEMPWOLFF Abstract.

More information

arxiv: v1 [astro-ph.sr] 26 Feb 2009

arxiv: v1 [astro-ph.sr] 26 Feb 2009 Baltic Astronomy, vol. 17, 293 (2008). MULTI-EPOCH UBVRcIc PHOTOMETRIC CATALOG OF SYM- BIOTIC STARS arxiv:0902.4604v1 [astro-ph.sr] 26 Feb 2009 Arne Henden 1 and Ulisse Munari 2 1 AAVSO, 49 Bay State Road,

More information

Studies of the Long Secondary Periods in Pulsating Red Giants. II. Lower- Luminosity Stars

Studies of the Long Secondary Periods in Pulsating Red Giants. II. Lower- Luminosity Stars Percy and Leung, JAAVSO Volume 45, 2017 1 Studies of the Long Secondary Periods in Pulsating Red Giants. II. Lower- Luminosity Stars John R. Percy Henry Wai-Hin Leung Department of Astronomy and Astrophysics,

More information

arxiv:astro-ph/ v1 30 Mar 2001

arxiv:astro-ph/ v1 30 Mar 2001 1 Detached Eclipsing Binaries for Parallax Measurements Irena S e m e n i u k Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland e-mail: is@astrouw.edu.pl ABSTRACT arxiv:astro-ph/0103511v1

More information

Chapter 30 Design and Analysis of

Chapter 30 Design and Analysis of Chapter 30 Design and Analysis of 2 k DOEs Introduction This chapter describes design alternatives and analysis techniques for conducting a DOE. Tables M1 to M5 in Appendix E can be used to create test

More information

I M P O R T A N T S A F E T Y I N S T R U C T I O N S W h e n u s i n g t h i s e l e c t r o n i c d e v i c e, b a s i c p r e c a u t i o n s s h o

I M P O R T A N T S A F E T Y I N S T R U C T I O N S W h e n u s i n g t h i s e l e c t r o n i c d e v i c e, b a s i c p r e c a u t i o n s s h o I M P O R T A N T S A F E T Y I N S T R U C T I O N S W h e n u s i n g t h i s e l e c t r o n i c d e v i c e, b a s i c p r e c a u t i o n s s h o u l d a l w a y s b e t a k e n, i n c l u d f o l

More information

Do Eclipsing Variable Stars Show Random Cycle-to-cycle Period Fluctuations?

Do Eclipsing Variable Stars Show Random Cycle-to-cycle Period Fluctuations? 80 Mohajerani and Percy, JAAVSO Volume 39, 2011 Do Eclipsing Variable Stars Show Random Cycle-to-cycle Period Fluctuations? Seyedyara Mohajerani John R. Percy Department of Astronomy and Astrophysics,

More information

Help parents get their kids settled in with this fun, easy-to-supervise coloring activity. A Fun Family Portrait... 3

Help parents get their kids settled in with this fun, easy-to-supervise coloring activity. A Fun Family Portrait... 3 K u R C d C! m m m k m u y g H p u R Cd C g d g b u d yu g p m d fu g f pg m g w Tk yu C g p D Ng kd pg u bk! T y g b fm dy m d md g g p By pvdg ud d ug yu u f D Ng Cg v, yu b pg up g u d g v bf W v pvdd

More information

Nearby Star Names: Cross Reference List

Nearby Star Names: Cross Reference List Nearby Star Names: Cross Reference List (1) Name. Usually a proper name or a distinctive catalog designation. Lists often vary regarding a "common" name. (2) Gliese-Jahreiss 3rd Catalong of Nearby Stars.

More information

The Light Curves Of RR Lyrae Field Stars

The Light Curves Of RR Lyrae Field Stars University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Norman R. Simon Papers Research Papers in Physics and Astronomy 10-15-1982 The Light Curves Of RR Lyrae Field Stars Norman

More information

Globular Clusters. This list contains 135 of the brightest and largest globular clusters from the Astroleague's observing program/list.

Globular Clusters. This list contains 135 of the brightest and largest globular clusters from the Astroleague's observing program/list. Globular Clusters A globular cluster is a spherical collection of stars that orbit a galactic core as a satellite. Globular clusters are very tightly bound by gravity, giving them their spherical shapes

More information

Binary star speckle measurements during from the SAO 6-m and 1-m telescopes in Zelenchuk

Binary star speckle measurements during from the SAO 6-m and 1-m telescopes in Zelenchuk ASTRONOMY & ASTROPHYSICS DECEMBER II 1999, PAGE 287 SUPPLEMENT SERIES Astron. Astrophys. Suppl. Ser. 140, 287 292 (1999) Binary star speckle measurements during 1992-1997 from the SAO 6-m and 1-m telescopes

More information

Made-to-measure malaria vector control strategies: rational design based on insecticide properties and coverage of blood resources for mosquitoes

Made-to-measure malaria vector control strategies: rational design based on insecticide properties and coverage of blood resources for mosquitoes J v DF. Fy f DF f x (HL) v w b vb. -- v g: g b vg f b f q J 2014, 13:146 :10.1186/1475-2875-13-146 Gy F K (gk@..z) k y (k@y.) J Gg (zg@.gv) Jf C v (jy.v@.g) C J Dky (.ky@..k) k C (k.@b.) 1475-2875 y vw

More information

Period study of the δ Scuti variable DE Lac

Period study of the δ Scuti variable DE Lac Bull. Astr. Soc. India (2014) 42, 19 25 Period study of the δ Scuti variable DE Lac S.-M. Wang, 1,2,3 S.-B. Qian, 1,2,3 W.-P. Liao, 1,2 J. Zhang, 1,2 X. Zhou, 1,2,3 and E.-G. Zhao 1,2 1 Yunnan Observatories,

More information

The Evolution of Outsourcing

The Evolution of Outsourcing Uvy f R I DCmm@URI S H Pj H Pm Uvy f R I 2009 T Ev f O M L. V Uvy f R I, V99@m.m Fw wk : ://mm../ P f B Cmm Rmm C V, M L., "T Ev f O" (2009). S H Pj. P 144. ://mm..//144://mm..//144 T A b y f f by H Pm

More information

CAT. NO /irtl,417~ S- ~ I ';, A RIDER PUBLICATION BY H. A. MIDDLETON

CAT. NO /irtl,417~ S- ~ I ';, A RIDER PUBLICATION BY H. A. MIDDLETON CAT. NO. 139-3 THIRD SUPPLEMENT I /irtl,417~ S- ~ I ';,... 0 f? BY H. A. MIDDLETON.. A RIDER PUBLICATION B36 B65 B152 B309 B319 B329 B719 D63 D77 D152 DA90 DAC32 DAF96 DC70 DC80 DCC90 DD6 DD7 DF62 DF91

More information

The TESS RR Lyrae and Cepheid Survey

The TESS RR Lyrae and Cepheid Survey The TESS RR Lyrae and Cepheid Survey Róbert Szabó 1, Katrien Kolenberg 2,3 (chairs) László Molnár 1, Emese Plachy 1, and TASC WG#6 1 Konkoly Observatory, MTA CSFK, Budapest, Hungary email: szabo.robert@csfk.mta.hu

More information

CH 61 USING THE GCF IN EQUATIONS AND FORMULAS

CH 61 USING THE GCF IN EQUATIONS AND FORMULAS CH 61 USING THE GCF IN EQUATIONS AND FORMULAS Introduction A while back we studied the Quadratic Formula and used it to solve quadratic equations such as x 5x + 6 = 0; we were also able to solve rectangle

More information

FAIR FOOD GRADE 8 SOCIAL STUDIES ICONIC EDIBLES LIGHTS CAMERA ACTION!

FAIR FOOD GRADE 8 SOCIAL STUDIES ICONIC EDIBLES LIGHTS CAMERA ACTION! FAIR FOO GRAE 8 SOCIA IES ICONIC EIBES IGHTS CAMERA ACTION! F F G Egh Icc Eb gh Cm Ac! I h w: cm c fm b q f h S F f Tx. Az h cb f v c hc gp. cb vpm h c h q Amc c. W, pc, cm b cc b f h Tx S F. m w f j v

More information

THE RELATIONSHIP BETWEEN THE COLOR AND LUMINOSITY OF STARS NEAR

THE RELATIONSHIP BETWEEN THE COLOR AND LUMINOSITY OF STARS NEAR THE RELATIONSHIP BETWEEN THE COLOR AND LUMINOSITY OF STARS NEAR THE SUN OLIN J. EGGEN LICK OBSERVATORY, UNIVERSITY OF CALIFORNIA The tabulation and description of all the individual stars was once considered

More information

Advanced Radiology Reporting and Analytics with rscriptor vrad results after 10 million radiology reports

Advanced Radiology Reporting and Analytics with rscriptor vrad results after 10 million radiology reports Av Ry R Ay wh vr 10 y I, w, v, - y y h, v, z yz y. I wh vy y v y hh-qy y z. A h h h N L P (NLP) h w y y. h w w vr Jy 2014 h h h 10 y. F h - w vr hv wk h v h qy wkw. h wh h h. I I /v h h wk wh vy y v w

More information

NVLAP Proficiency Test Round 14 Results. Rolf Bergman CORM 16 May 2016

NVLAP Proficiency Test Round 14 Results. Rolf Bergman CORM 16 May 2016 NVLAP Proficiency Test Round 14 Results Rolf Bergman CORM 16 May 2016 Outline PT 14 Structure Lamp Types Lab Participation Format for results PT 14 Analysis Average values of labs Average values of lamps

More information

Intrinsic variable types on the Hertzsprung Russell diagram. Image credit: Wikipedia

Intrinsic variable types on the Hertzsprung Russell diagram. Image credit: Wikipedia Studying intrinsically pulsating variable stars plays a very important role in stellar evolution understanding. The Hertzsprung-Russell diagram is a powerful tool to track which stage of stellar life is

More information

S n+1 (1 + r) n+1 S ] (1 + r) n + n X T = X 0 + ( S) T,

S n+1 (1 + r) n+1 S ] (1 + r) n + n X T = X 0 + ( S) T, (S K) + (S K) + (S K) + (X 0 0 S 0, 0 S 0 ) X 0 0 (X 0 0 S 0 ) X 0 ( + r)(x 0 0 S 0 ) + 0 S (S K) +. S (H) us 0 S (T ) ds 0 X 0 0 u d X 0.0 0 (S K) + ( X 0 + 0 S 0, 0 S 0 ) 0 0 S 0 X 0 X 0 C 0 X 0 C 0

More information

Chemistry 2 Exam Roane State Academic Festival. Name (print neatly) School

Chemistry 2 Exam Roane State Academic Festival. Name (print neatly) School Name (print neatly) School There are fifteen question on this exam. Each question is weighted equally. n the answer sheet, write your name in the space provided and your answers in the blanks provided.

More information

GUIDE. mirfieldshow.com. Sponsored by. Orange Design Studio.

GUIDE. mirfieldshow.com. Sponsored by. Orange Design Studio. GUIDE mfhw.m Sp b O D S. Fh F m F C 1 3 5 7 9 b f M MIRFIELD COAT OF ARMS Th m w ff Fb 26, 1935. Th m f h mp f h w m h m. Th p S Jh H, wh pp h Pp h 13h h b f h ph hh. Hv W H Wh h? O, h wm mh, hp h f h.

More information

arxiv: v1 [astro-ph.sr] 27 Sep 2017

arxiv: v1 [astro-ph.sr] 27 Sep 2017 Amplitude Variations in Pulsating Red Giants. II. Some Systematics arxiv:1709.09696v1 [astro-ph.sr] 27 Sep 2017 John R. Percy Department of Astronomy and Astrophysics, and Dunlap Institute of Astronomy

More information

Catalog Information and Recommendations

Catalog Information and Recommendations Catalog Information and Recommendations U.S. Naval Observatory, December, 2000 P.O.C. Sean Urban (seu@pyxis.usno.navy.mil) 1 Introduction The following is a list of widely used or well known catalogs for

More information

A METHOD OF COLOR EXCESS DETERMINATION FOR HIGH AMPLITUDE δ SCUTI STARS

A METHOD OF COLOR EXCESS DETERMINATION FOR HIGH AMPLITUDE δ SCUTI STARS Journal of The Korean Astronomical Society 42: 155 159, 2009 December c 2009 The Korean Astronomical Society. All Rights Reserved. A METHOD OF COLOR EXCESS DETERMINATION FOR HIGH AMPLITUDE δ SCUTI STARS

More information

Chair Susan Pilkington called the meeting to order.

Chair Susan Pilkington called the meeting to order. PGE PRK D RECREO DVOR COMMEE REGUR MEEG MUE MOD, JU, Ru M h P P d R d Cmm hd : m Ju,, h Cu Chmb C H P, z Ch u P dd, Mmb B C, Gm Cu D W Bd mmb b: m D, d Md z ud mmb : C M, J C P Cmmu Dm D, Km Jh Pub W M,

More information

Mathematics Course 111: Algebra I Part I: Algebraic Structures, Sets and Permutations

Mathematics Course 111: Algebra I Part I: Algebraic Structures, Sets and Permutations Mathematics Course 111: Algebra I Part I: Algebraic Structures, Sets and Permutations D. R. Wilkins Academic Year 1996-7 1 Number Systems and Matrix Algebra Integers The whole numbers 0, ±1, ±2, ±3, ±4,...

More information

7.2. Matrix Multiplication. Introduction. Prerequisites. Learning Outcomes

7.2. Matrix Multiplication. Introduction. Prerequisites. Learning Outcomes Matrix Multiplication 7.2 Introduction When we wish to multiply matrices together we have to ensure that the operation is possible - and this is not always so. Also, unlike number arithmetic and algebra,

More information

Studies of Peculiar Black Holes with Gemini Telescopes

Studies of Peculiar Black Holes with Gemini Telescopes Studies of Peculiar Black Holes with Gemini Telescopes Minjin Kim (KASI) In collaboration with Luis Ho (KIAA), Myungshin Im (Seoul National University), Peter Jonker (SRON), Francesca Onori (SRON) Contents

More information

Characterization of variable stars using the ASAS and SuperWASP databases

Characterization of variable stars using the ASAS and SuperWASP databases Characterization of variable stars using the ASAS and SuperWASP databases Derck P. Smits Dept of Mathematical Sciences, PO Box 392, UNISA, 0003, South Africa E-mail: smitsdp@unisa.ac.za Abstract. A photographic

More information

Contents FREE!

Contents FREE! Fw h Hu G, h Cp h w bu Vy Tu u P. Th p h pk wh h pp h. Th u y D 1 D 1 h h Cp. Th. Th hu K E xp h Th Hu I Ch F, bh K P pp h u. Du h p, K G u h xp Ch F. P u D 11, 8, 6, 4, 3. Th bk w K pp. Wh P p pp h p,

More information

Stellar classification by means of CCD spectrography

Stellar classification by means of CCD spectrography Stellar classification by means of CCD spectrography by M.M.M. Santangelo 1,2 & M. Pasquini 1,2 1 I.R.F. Istituto Ricerche Fotometriche (LU), Italy 2 O.A.C. Osservatorio Astronomico di Capannori (LU) Instruments

More information

I N A C O M P L E X W O R L D

I N A C O M P L E X W O R L D IS L A M I C E C O N O M I C S I N A C O M P L E X W O R L D E x p l o r a t i o n s i n A g-b eanste d S i m u l a t i o n S a m i A l-s u w a i l e m 1 4 2 9 H 2 0 0 8 I s l a m i c D e v e l o p m e

More information

2 u Du, k Hu Dv Hu, y H. u Cu j u qu u. Nv. v uy. Cu Hu F A H. qu Cu.. Cu j 1980, u V, v Nu My O k. v u u. A G C. My u v k, 2.5 H v v u / u v u v k y

2 u Du, k Hu Dv Hu, y H. u Cu j u qu u. Nv. v uy. Cu Hu F A H. qu Cu.. Cu j 1980, u V, v Nu My O k. v u u. A G C. My u v k, 2.5 H v v u / u v u v k y H HE 1016 M EEING OF HE ODIE CLU 1,016 Cu 7:30.. D 11, 2007 y W L Uvy. C : Pu A y: Ov 25 x u. Hk, u k MA k D u y Hu, u G, u C C, MN C, Nk Dv Hu, MN, u K A u vu v. W y A Pku G, G u. N EW UINE: D, Cu, 22

More information

VERY LARGE ARRAY PLUS PIE TOWN ASTROMETRY OF 46 RADIO STARS

VERY LARGE ARRAY PLUS PIE TOWN ASTROMETRY OF 46 RADIO STARS The Astronomical Journal, 133:906Y 916, 2007 March # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. VERY LARGE ARRAY PLUS PIE TOWN ASTROMETRY OF 46 RADIO STARS D. A. Boboltz,

More information

100Z-1 100Z-1 51 HA 50. Cushion ring Cushion ring. Type. Standard type. Switch Set

100Z-1 100Z-1 51 HA 50. Cushion ring Cushion ring. Type. Standard type. Switch Set 0Z-1 0Z-1 51 Type Nominal pressure Maximum allowable pressure Proof test pressure Minimum operating pressure Working speed range Working temperature range (ambient/fluid temperature) Structure of cushioning

More information

H STO RY OF TH E SA NT

H STO RY OF TH E SA NT O RY OF E N G L R R VER ritten for the entennial of th e Foundin g of t lair oun t y on ay 8 82 Y EEL N E JEN K RP O N! R ENJ F ] jun E 3 1 92! Ph in t ed b y h e t l a i r R ep u b l i c a n O 4 1922

More information

106 70/140H-8 70/140H-8

106 70/140H-8 70/140H-8 7/H- 6 H 7/H- 7 H ffffff ff ff ff ff ff ff ff ff f f f f f f f f f f f ff f f f H 7/H- 7/H- H φφ φφ φφ φφ! H 1 7/H- 7/H- H 1 f f f f f f f f f f f f f f f f f f f f f f f f f f f f f ff ff ff ff φ φ φ

More information

UCM DEPARTMENT OF THEATRE & DANCE PRESENTS SEASON

UCM DEPARTMENT OF THEATRE & DANCE PRESENTS SEASON UCM DEPARTMENT OF THEATRE & DANCE PRESENTS BECOME A SEASON SUBSCRIBER! Dh m wh ym : UCM Dm f Th D Uvy f C M PO Bx 800 M 113 Wbg, MO 64093 A Cv Sy M A bb, y y k F bf h bx ff. T v y k f F g wh y k, h f h

More information

Whitney Grummon. She kick started a fire in my soul Teaching me a tool to cleanse my mind That ll last a life time. That s how I will remember

Whitney Grummon. She kick started a fire in my soul Teaching me a tool to cleanse my mind That ll last a life time. That s how I will remember W Gmm S kk f m T m m m T f m T I mmb N m p f p f f G L A f b k, b k v M k b p:, bb m, m f m, v. A b m, f mm mm f v b G p. S m m z pp pv pm f, k mk, f v M. I m, I m, fm k p x. S f 45 m m CMS, I p mf,. B

More information

5 H o w t o u s e t h e h o b 1 8

5 H o w t o u s e t h e h o b 1 8 P l a s r a d h i s m a n u a l f i r s. D a r C u s m r, W w u l d l i k y u bb a si n p r hf r m a n cf r m y u r p r d u c h a h a s b n m a n u f a c u r d m d r n f a c i l iu n id s r s r i c q u

More information

Does the Period of a Pulsating Star Depend on its Amplitude?

Does the Period of a Pulsating Star Depend on its Amplitude? Percy and Yook, JAAVSO Volume 42, 2014 245 Does the Period of a Pulsating Star Depend on its Amplitude? John R. Percy Jeong Yeon Yook Department of Astronomy and Astrophysics, University of Toronto, Toronto,

More information

I n t e r n a t i o n a l E l e c t r o n i c J o u r n a l o f E l e m e n t a r y E.7 d u, c ai ts is ou n e, 1 V3 1o-2 l6, I n t h i s a r t

I n t e r n a t i o n a l E l e c t r o n i c J o u r n a l o f E l e m e n t a r y E.7 d u, c ai ts is ou n e, 1 V3 1o-2 l6, I n t h i s a r t I n t e r n a t i o n a l E l e c t r o n i c J o ue rlne am l e not fa r y E d u c a t i o n, 2 0 1 4, 1 37-2 ( 16 ). H o w R e a d i n g V o l u m e A f f e c t s b o t h R e a d i n g F l u e n c y

More information

D ON MY HONOR, I WILL TRY.. AISI S E R S O DASS A B BR AM OWNI S E R S I GIRL SCOUTS! JUN SENIO IORS CAD E TTES

D ON MY HONOR, I WILL TRY.. AISI S E R S O DASS A B BR AM OWNI S E R S I GIRL SCOUTS! JUN SENIO IORS CAD E TTES ON MY HONOR, I WILL TRY.. DAISI ES AMBASSADORS BROWNI ES I JUNIORS 2017-2018 GIRL SCOUTS! CAD E TTES SENIORS Wm! W' I? W'v Pm G, v, m m G S x. I, y' m w x m, v, v v G S G W M. T v wm.. I y v y q q m, 888.474.9686

More information

Evaluation of The Necessary of Agriculture Public Expenditure for Poverty Reduction and Food Security in Benin

Evaluation of The Necessary of Agriculture Public Expenditure for Poverty Reduction and Food Security in Benin MPRA Mu P RPE Av Evu N Aguu Pu Exu Pv Ru F Su B A C L Zg Uv E Lw O 010 O ://.u.u-u./447/ MPRA P N. 447, 7. Augu 010 0:17 UC qwugjkzxvqw ugjkzxvqwu gjkzxvqwug [ Evu N jkzxvqwugjkzx vqwugjkzxv qwugjkzxvqw

More information

FICH~:s lciithyo\l~~trio~es.

FICH~:s lciithyo\l~~trio~es. PB FCNyM UNLP T g vg wk b b y y g b y F wk v b m b v gz w my y m g E bv b g y v q y q q ó y P mv gz y b v m q m mó g FCH CTHYOTROES P W P -C b } k < HP- qe q< - - < - m T

More information

Baltic Astronomy, vol. 23, , 2014 OBSERVATIONS OF TWO UNUSUAL ECLIPSING BINARIES, FN CAM AND AG VIR

Baltic Astronomy, vol. 23, , 2014 OBSERVATIONS OF TWO UNUSUAL ECLIPSING BINARIES, FN CAM AND AG VIR Baltic Astronomy, vol. 23, 255 259, 2014 OBSERVATIONS OF TWO UNUSUAL ECLIPSING BINARIES, FN CAM AND AG VIR E. A. Avvakumova 1, O. Yu. Malkov 2, A. A. Popov 1 and A. Yu. Kniazev 3,4,5 1 Kourovka Astronomical

More information

GNSS-Based Orbit Determination for Highly Elliptical Orbit Satellites

GNSS-Based Orbit Determination for Highly Elliptical Orbit Satellites -Bd D f Hghy p Q,*, ug, Ch Rz d Jy u Cg f u gg, g Uvy f u d u, Ch :6--987, -:.q@ud.uw.du. h f uvyg d p If y, Uvy f w uh W, u : h Hghy p H ufu f y/yhu f h dgd hv w ud pg h d hgh ud pg h f f h f. Du h g

More information

Messier Marathon Checkoff List 1

Messier Marathon Checkoff List 1 Messier Marathon Checkoff List 1 by Ken Graun DATE 8 p.m. 2 74 3, 77, 52, 31/32/110, 33, 103, 111/112, 76, 34 M74 1h 36.7m +15 47' Psc Spiral Galaxy 9.2 10' x 9' The Phantom M77 2h 42.7m 0 01' Cet Spiral

More information

THIS PAGE DECLASSIFIED IAW E

THIS PAGE DECLASSIFIED IAW E THS PAGE DECLASSFED AW E0 2958 BL K THS PAGE DECLASSFED AW E0 2958 THS PAGE DECLASSFED AW E0 2958 B L K THS PAGE DECLASSFED AW E0 2958 THS PAGE DECLASSFED AW EO 2958 THS PAGE DECLASSFED AW EO 2958 THS

More information

N C GM L P, u u y Du J W P: u,, uy u y j S, P k v, L C k u, u GM L O v L v y, u k y v v QV v u, v- v ju, v, u v u S L v: S u E x y v O, L O C u y y, k

N C GM L P, u u y Du J W P: u,, uy u y j S, P k v, L C k u, u GM L O v L v y, u k y v v QV v u, v- v ju, v, u v u S L v: S u E x y v O, L O C u y y, k Qu V vu P O B x 1361, Bu QLD 4575 C k N 96 N EWSLEE NOV/ DECE MBE 2015 E N u uu L O C 21 Nv, 2 QV v Py Cu Lv Su, 23 2 5 N v, 4 2015 u G M v y y : y quu u C, u k y Bu k v, u u vy v y y C k! u,, uu G M u

More information

Discovery Guide. Beautiful, mysterious woman pursued by gunmen. Sounds like a spy story...

Discovery Guide. Beautiful, mysterious woman pursued by gunmen. Sounds like a spy story... Dv G W C T Gp, A T Af Hk T 39 Sp. M Mx Hk p j p v, f M P v...(!) Af Hk T 39 Sp, B,,, UNMISSABLE! T - f 4 p v 150 f-p f x v. Bf, k 4 p v 150. H k f f x? D,,,, v? W k, pf p f p? W f f f? W k k p? T p xp

More information

Observing Stellar Evolution Observing List

Observing Stellar Evolution Observing List Observing Stellar Evolution Observing List Bill Pellerin, Houston Astronomical Society This list is organized by category of object. Within each category, the list is sorted by RA to help you plan your

More information

Rømer Science Mission Plan

Rømer Science Mission Plan Institute of Physics and Astronomy, University of Aarhus Rømer Science Mission Plan Danish Small Satellite Programme Document No.(issue): MONS/IFA/MAN/PLN/0001(1) Date: 2001-05-29 Prepared by: Jørgen Christensen-Dalsgaard,

More information

Symbolising Quantified Arguments

Symbolising Quantified Arguments Symbolising Quantified Arguments 1. (i) Symbolise the following argument, given the universe of discourse is U = set of all animals. Animals are either male or female. Not all Cats are male, Therefore,

More information

Lab Day and Time: Instructions. 1. Do not open the exam until you are told to start.

Lab Day and Time: Instructions. 1. Do not open the exam until you are told to start. Name: Lab Day and Time: Instructions 1. Do not open the exam until you are told to start. 2. This exam is closed note and closed book. You are not allowed to use any outside material while taking this

More information

:,,.. ;,..,.,. 90 :.. :, , «-»,, -. : -,,, -, -., ,, -, -. - «-»:,,, ,.,.

:,,.. ;,..,.,. 90 :.. :, , «-»,, -. : -,,, -, -., ,, -, -. - «-»:,,, ,.,. .,.,. 2015 1 614.8 68.9 90 :,,.. ;,. 90.,.,. :.. :, 2015. 164. - - 280700, «-»,, -. : -,,, -, -.,. -. -. -,, -, -. - «-»:,,, -. 614.8 68.9.,.,., 2015, 2015 2 ... 5... 7 1.... 7 1.1.... 7 1.2.... 9 1.3....

More information

ATTACHMENT 10 WRITTEN DIRECT NOTICE TO ELECTRIC UTILITIES WITHIN FIVE MILES

ATTACHMENT 10 WRITTEN DIRECT NOTICE TO ELECTRIC UTILITIES WITHIN FIVE MILES AACHMEN 10 WIEN DIEC NOICE O ELEIC UILIIE WIHIN FIVE MILE 1087 his page left blank intentionally. 1088 ELEIC UILIIE O ECEIVE NOICE AACHMEN 10 Utility Aress City tate Zip Coe AEP exas Central Co. 539 N.

More information

What is the periodic table?

What is the periodic table? The periodic table of the elements represents one of the greatest discoveries in the history of science that certain elements, the basic chemical substances from which all matter is made, resemble each

More information

A note on the acyclic 3-choosability of some planar graphs

A note on the acyclic 3-choosability of some planar graphs A note on the acyclic 3-choosability of some planar graphs Hervé Hocquard, Mickael Montassier, André Raspaud To cite this version: Hervé Hocquard, Mickael Montassier, André Raspaud. A note on the acyclic

More information

Secondary Support Pack. be introduced to some of the different elements within the periodic table;

Secondary Support Pack. be introduced to some of the different elements within the periodic table; Secondary Support Pack INTRODUCTION The periodic table of the elements is central to chemistry as we know it today and the study of it is a key part of every student s chemical education. By playing the

More information

R a. Aeolian Church. A O g C. Air, Storm, Wind. P a h. Affinity: Clan Law. r q V a b a. R 5 Z t 6. c g M b. Atroxic Church. d / X.

R a. Aeolian Church. A O g C. Air, Storm, Wind. P a h. Affinity: Clan Law. r q V a b a. R 5 Z t 6. c g M b. Atroxic Church. d / X. A M W A A A A R A O C A () A 6 A A G A A A A A A-C Au A A P 0 V A T < Au J Az01 Az02 A Au A A A A R 5 Z 6 M B G B B B P T Bu B B B B S B / X B A Cu A, S, W A: S Hu Ru A: C L A, S, F, S A, u F C, R C F

More information

C o r p o r a t e l i f e i n A n c i e n t I n d i a e x p r e s s e d i t s e l f

C o r p o r a t e l i f e i n A n c i e n t I n d i a e x p r e s s e d i t s e l f C H A P T E R I G E N E S I S A N D GROWTH OF G U IL D S C o r p o r a t e l i f e i n A n c i e n t I n d i a e x p r e s s e d i t s e l f i n a v a r i e t y o f f o r m s - s o c i a l, r e l i g i

More information

o C *$ go ! b», S AT? g (i * ^ fc fa fa U - S 8 += C fl o.2h 2 fl 'fl O ' 0> fl l-h cvo *, &! 5 a o3 a; O g 02 QJ 01 fls g! r«'-fl O fl s- ccco

o C *$ go ! b», S AT? g (i * ^ fc fa fa U - S 8 += C fl o.2h 2 fl 'fl O ' 0> fl l-h cvo *, &! 5 a o3 a; O g 02 QJ 01 fls g! r«'-fl O fl s- ccco > p >>>> ft^. 2 Tble f Generl rdnes. t^-t - +«0 -P k*ph? -- i t t i S i-h l -H i-h -d. *- e Stf H2 t s - ^ d - 'Ct? "fi p= + V t r & ^ C d Si d n. M. s - W ^ m» H ft ^.2. S'Sll-pl e Cl h /~v S s, -P s'l

More information

o Alphabet Recitation

o Alphabet Recitation Letter-Sound Inventory (Record Sheet #1) 5-11 o Alphabet Recitation o Alphabet Recitation a b c d e f 9 h a b c d e f 9 h j k m n 0 p q k m n 0 p q r s t u v w x y z r s t u v w x y z 0 Upper Case Letter

More information

Ninth Marine Air Wing To Be Decommissioned. ment of the Transport Air Broup.

Ninth Marine Air Wing To Be Decommissioned. ment of the Transport Air Broup. N M W T B D $ R V /RNE M N 2 C O R R & F O T T O O N T TTON-CHERRY ONT NC B D OM O z C M H N M W O z M 944 T W ; N W j j C T q T N W T W z ; q q z - M 30 946 F T G O R [MR 252952 C q -C - T G VMR 252 V

More information

I zm ir I nstiute of Technology CS Lecture Notes are based on the CS 101 notes at the University of I llinois at Urbana-Cham paign

I zm ir I nstiute of Technology CS Lecture Notes are based on the CS 101 notes at the University of I llinois at Urbana-Cham paign I zm ir I nstiute of Technology CS - 1 0 2 Lecture 1 Lecture Notes are based on the CS 101 notes at the University of I llinois at Urbana-Cham paign I zm ir I nstiute of Technology W hat w ill I learn

More information

electronic reserve R regular reserve: required background reading for those without background in early China Course introduction 1/20

electronic reserve R regular reserve: required background reading for those without background in early China Course introduction 1/20 PHILOSOPHICAL MASTERS OF ANCIENT CHINA P T A W O: KJ 128 O : M 4-5; W 2-3 Hy 333 Spg 2004 C : TR 10:30-11:45 C : CUPR 203 Rq x p: T A C A Wy (Vg Bk 1938; Rp ) M DC L (Pg C Vkg P; Rp ) T C Wy V: T g Lz

More information

Analysis of Collaborative Learning Behaviors and the Roles of Collaborative Learning Agent

Analysis of Collaborative Learning Behaviors and the Roles of Collaborative Learning Agent A v L Bhv h v L A Ik L (Sj Uv, S. K, @j..k) J H L (Uv Ih, S. K, jh@h..k) Sh J (S N Uv, S. K, v712@..k) E M S (S N Uv, S. K, 04@..k) K A M (E T h I, S. K, k@..k) H J S (E T h I, S. K, hjh@..k) A: v h h

More information

Variable star light curve activity

Variable star light curve activity Variable star light curve activity 2013. All rights reserved. SPIRIT is based at The University of Western Australia. 2016. All rights reserved. SPIRIT is based at The University of Western Australia 2

More information

Created by T. Madas MIXED SURD QUESTIONS. Created by T. Madas

Created by T. Madas MIXED SURD QUESTIONS. Created by T. Madas MIXED SURD QUESTIONS Question 1 (**) Write each of the following expressions a single simplified surd a) 150 54 b) 21 7 C1A, 2 6, 3 7 Question 2 (**) Write each of the following surd expressions as simple

More information

CHEM 10113, Quiz 5 October 26, 2011

CHEM 10113, Quiz 5 October 26, 2011 CHEM 10113, Quiz 5 October 26, 2011 Name (please print) All equations must be balanced and show phases for full credit. Significant figures count, show charges as appropriate, and please box your answers!

More information

Pulsation Properties of Carbon and Oxygen Red Giants

Pulsation Properties of Carbon and Oxygen Red Giants Percy and Huang, JAAVSO Volume 43, 2015 1 Pulsation Properties of Carbon and Oxygen Red Giants John R. Percy Danping Joanna Huang Department of Astronomy and Astrophysics, University of Toronto, Toronto,

More information

Fuzzy Reasoning and Optimization Based on a Generalized Bayesian Network

Fuzzy Reasoning and Optimization Based on a Generalized Bayesian Network Fuy R O B G By Nw H-Y K D M Du M Hu Cu Uvy 48 Hu Cu R Hu 300 Tw. @w.u.u.w A By w v wy u w w uy. Hwv u uy u By w y u v w uu By w w w u vu vv y. T uy v By w w uy v v uy. B By w uy. T uy v uy. T w w w- uy.

More information