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1 Abell clusters, -- distance groups of -- radio sources and -- richness of - A 194,400,1314 -A A A A A A A 2670 absorption line spectra (radio galaxies) " "systems (quasars) ,71 69,71, ,46-48, acceleration of particles, mechanisms -- in conducting fluids --- in fluids with reduced conductivity --- by pulsars ---- by supernovae --- in extragalactic radio sources ,179, ,96,100,108,112 accretion, disk --- gravitational energy release from --- in close binaries adiabatic compression --- losses "after-burner" effect A1fven waves, Fermi acceleration by Algol 99,117, , , ,238, , 255, , G. Setti (ed.), The Physics of Non-Thermal Rodio Sources, All Rights Reser"ed by D. Reidel Publishing Comptlny, Dordrecht-Hollllnd.
2 272 alignment of components, ---- with galaxy rotational axes angular resolution angular size-flux density relation " "-redshift " " " of compact sources aperture synthesis 31,32,34,39, , , Balmer decrement baseline, projected beam, synthesized --- primary Bernouilli equation betatron acceleration binary stars, X-ray emission from ---- radio emission from "normal" black-body, X-ray emission from black hole blast wave, relativistic BL Lac BL Lac objects, ---- AP Lib AO bremsstrahlung, thermal brightness temperature limit " " in compact sources BSO 6 B , ,233, ,247, ,117,238,239,247, ,35, ,119, , , ,36 31,36,
3 Cancer cluster Canis Minoris Cas A Capella "cavity", in extragalactic radio sources ----, energy content of cd galaxies " clusters Cen X-3 "Christmas tree" model clusters of galaxies ---- Bautz-Morgan scheme of ---- galaxy types in ---- galaxy types distribution in ---- gravitational binding of ---- gravitational radius of ---- Rood-Sastry scheme of ---- types of ---- Zwicky "cocoon", extragalactic r.s. coherence length coherent objects, ejection of coherent processes Coma cluster, compact nuclear components; see compact radio sources ,144,198,199, ,97,99 96,97 42,69,72,74 70,72 235, , ,70 70, , ,70 72,76,77, ,109, ,61,113,116,185 70,71,74,76 264, compact radio sources, ---- energy content of ---- expansion model of ---- magnetic field strength in ---- radiation mechanisms in 12,15,16,19,27-39,99, ,127,128 31,117,127, ,32 116
4 274 "composite average" QSO spectrum 59 compton scattering " "cooling " "losses continental drift convection, compression by cooling time Coronae Borealis cluster coronas of stars, X-ray emission from cosmic rays, confinement of ---- energy density of ---- lifetime of ---- from supernovae Crab Nebula 61,94,97,116,127, , ,175, , ,145, ,164 45,153,161,185, , 229,243,262,263 Crab Nebula pulsar; see NP 0531 CTA 102 Cygnus A Cyg X-1 Cyg X-2 Cyg X ,32,44,46,50,51, 95-97,100,112,113, ,210, ,232,240, , ,210,229,247, ,210, ,254 DA 240 D galaxies (definition) dispersion measure double double radio sources double radio sources, assymmetric ---- beam model of ---- collimated ~
5 double radio sources, inside and outside clusters ---- symmetric relaxed "dumbbell" galaxies dust features, peculiar -- lane dynamic range 73 16,17, ,49 6, Earth axis " magnetosphere Eddington limit electron radiative lifetimes, in Crab in head tails in hot spots in QSOs elliptical galaxies (giant) emission line spectra (radio galaxies) " " " (quasars) emission measure energy (beaming of) in radio sources expansion losses " model ", relativistic ", slowing down of extinction extragalactic radio sources, --- age of -- complex structures --- confinement of --- double structure -- energy requirements --- energy supply -- extended lobes properties -- head tail structure -- magnetic field structure in -- models of , 234, ,243,262 19, , , , ,38,61,115,127 94, ,23 67,76,94-97, ,94, ,14,96, ,14,16,19,
6 276 extragalactic radio sources, ---- morphological classification ---- physical parameters ---- power 10ff 7,8 11 Faraday rotation 14,95,100 Fermi acceleration, ---- in the Galaxy ---- in supernova remnants fine structure levels flow-pattern fluidized beds Fokker-Planck equation Fornax A Fourier transform 4C C free-free absorption (QSOs) 137,138, ,161 63,64 101, , ,16 3,4, galactic magnetic field, ---- buoyancy of ---- confinement of ---- instability of ---- origin of ---- strength galactic X-ray sources, luminosity of ---- number of y-ray bursts galaxies, collision of geomagnetic tail globular clusters, , , , , ,
7 globular clusters, X-ray bursts from -- NGC NGC NGC 6441,7078 (-M15) grating rings gridding GX 17+2 gyroradius , , "heads" of radio components "head-tail" structure Hercules cluster 95-97, ,101 70,71 Her X-I hot spots Hubble expansion ---- diagram for 3C radio galaxies HZ 43 HZ Her 235,249;250, , ,24,108,109,112, , IC 310 interference fringes interferometry, ---- long baseline interferometer polar diagram intergalactic matter, ---- ram pressure by interplanetary scintillation intrac1uster gas 77, ff 29, ,100,101,108,109 97, ,73-77
8 278 intrac1uster gas, ---- density of ---- parameters of (from head tail sources) ---- temperature ,260 97,234 interstellar gas, accretion of ---- dens i ty of ---- dispersion measure of ---- turbulence of ionized hydrogen in clusters , ,145,170,171,176 76,77 jets, - stability of 45,50,101,102, Kelvin-Helmholtz instability Kreminsky star 102, line-locking process log N-log S relationship, for 3C radio galaxies ---- for X-ray sources low-frequency e.m. waves, ---- acceleration by luminosity difference (due to Doppler shift) luminosity function, of galaxies in clusters of radio galaxies lunar occultation 63 85,90, ,234,236 95, , Mage11anic Clouds magnetic field, amplification of ---- in the Galaxy magnetospheric model ,21
9 map distortions " cleaning Markarian 231 matter density in radio components ", ejection of " flow in quasars M 87 " jet MCG molecular hydrogen, in clusters M super-giants, radio emission from M , ,95,125 63,64 32,47,49 47,49,50,100, neutral hydrogen, in clusters in elliptical galaxies neutral sheet reconnection, ---- particle acceleration by 74, neutron star (spinning) N galaxies (definition) NGC 55,300 NGC 541,545,547 NGC 1068 NGC 1265 NGC 1275 (=Per A) NGC 4151 NGC NGC 4874 NGC 5128 (=Cen A) 161,163, ,200,235, ,77, , 3 3, 5 1, 7 7 ~ 8 0, ,47, ,32,47-49,97.100,117,125, 132,234
10 280 NGC 5128 (=Cen A), X-ray emission from NGC 7720 noise limited novae, radio emission from Nova Del 1967 Ser 1970 Scuti 1970, symbiotic (R Agr) 236, nozzle, collimation by instability at NP 0531 nuclear activity nuclear burning, energy from 94,95,101,108, ,181,184,186,187,243,244 15,19,21,23,31,45,93-95, 97,107,109,112, , 125,127,128, ,242 OJ 287 oscillator strength 32,56,58 64 P Cygni profile "peculiar" galaxies (definition) Pegasus I cluster Perseus cluster phase information photo-electric absorption (X-rays) PKS plasma turbulence polarization, radio, optical (QSOs) polar motion ,23,74,77-80,126,234 29,30 263, ,145, ,164, ,
11 potential double layer PSR PSR PSR PSR PSR pulsars, age of ---- braking index of ---- brightness of ---- distances of ---- duty cycle of ---- emission mechanisms of ---- "glitches" of ---- in binary stars ---- magnetic field decay of ---- models of ---- optical emission from ---- period distribution of ---- polarization of ---- pulse shape ---- slowing down of ---- SN remnants and ---- x- and Y-ray emission from 138, , , , , , , , ,187,194,255, quasars, absorption lines in --- absorption line redshifts of --- abs. lines from intervening galaxies ---- absorption line region in --- color of --- continuum energy --- distance of -- D2 type --- electron density in --- emission lines of --- emission line models " "redshifts " "region -- energy production " requirements --- local --- optical appearance ---- polarization 57,59-61,63 57,60, ,58 57,58 61, , , ,128 56,57 57,58
12 282 quasars, variability PHL PHL PHL PKS PKS RS 23 57,58 234, ,62 61, radiation damping profile " pressure, acceleration from radio binaries ("normal") radio bridges (head-nuc1eus) radio galaxies, absorption lines from ---- and cosmology ---- emission lines from ---- morphology of ---- optical properties of ---- spectra of CR catalogue and ---- velocity fields in radio luminosity function, bivariate ---- forms of ---- from radio catalogues ---- from optical samples ---- inside and outside clusters ---- linear size correlation ---- structure form correlation 61, , ,112 44,46,47 52,53,85, ,44, ,234 51,52 89, , radio sources, identification of ---- parameters of ---- steep spectra radio stars, ----magnetic field in radio trail hypothesis Rayleigh-Taylor instability 24,44-48, , ,19,76,
13 recombination lines reddening redshift of quasars " systems in quasars resolution ellipse Roche lobes rotating magnetic dipole rotational axis (nuclei) " "alignment " " precession relativistic plasma, gradual production of ---- sudden production of ,56,61, , ,164, , ,17,19, Schwartzschild radius scintillation Sco X-I Sculptor group Seyfert galaxies, shear layer side lobes Sirius "sling-shot" model SMC X-I solar flare S-shape symmetry Stokes parameters "superluminous" velocities ,227, , , ,99 235, ,150,161,164 14,16,17, ,39,114,116
14 284 supermassive rotators 134,135 supernova energy production " explosion supernovae remnants, -- age of --- distances of --- expansion of ---- E-R relation synchro-compton radiation synchrotron emission ---- lifetime --- losses, s.pectra1 bend from SO galaxies, --- in clusters 131,134, ,161,232,239,242, , , , , , "tails" tearing instability 3C sources, -- in clusters identified with galaxies 3C 9 3C 33 3C 40,303 3C 47 3C 48 3C 66 3C 69,61.1,86A,184.1,285,336,430,452 3C 79,268.2,284,452 3C 84 3C 94,371 99, , , ,17 55, ,23,33,37 123
15 3C 109 3C 111 3C 120 3C 129 3C 147,154 3C 191 3C ,33,113 37,39,43 11,17,18,20, ,63,64 14, C 236 3C 273 " B " jet 3C 278 3C 286 3C 295 3C 310 3C 315,386 3C 345 3C C 430 3C 446 3C C 465 transient X-ray sources, low latitude -- high 1a ti tude -- A A U , , , U (= NAB , possible QSO) 12,15,17,21,97,108,112,113 24,37,39,55,56,62,128,131, 132,234, ,100, ,58,59 14,51,97, ,36,127 22,97 235, ,
16 286 3U (= A 478), (= A 2142) 3U (binary) 3U (binary) Ton 1530 "twin exhaust" model, -- evidence of Tycho SR , , UHURU X-ray observatory " catalogue UV Cety flare stars U-V plane 229, , ,29,30 variability, optical of quasars -- radio velocity discontinuity " fields in galaxies " of expansion " of outflow "violent event" Virgo A Virgo cluster Virial mass " theorem " velocities 58 34ff , ,48,49 16,49,97 70,234 76, VLBI vortex sheet 29,30,36,94, ,103 white dwarf, gravitational energy from -- X-ray from , X-ray background 234,235
17 X-ray clusters, radio properties of galaxy distribution in emission processes sources, low galactic latitude ", high" " ", energy source stars, magnetic field in radio emission from , ,232, ,215, ,
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