The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE
|
|
|
- June Paul
- 5 years ago
- Views:
Transcription
1 Characteristics VLT/NACO observations VLT/SPHERE observations Open questions The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE M. Montargès (IRAM), P. Kervella (CNRS/U. de Chile UMI FCA), E. Lagadec (Lagrange), S. T. Ridgway (NOAO), and many others... Stellar End Product: The Low Mass - High Mass Connection ESO Garching - July 8th 2015 M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 1/14
2 L2 Puppis ID card (ESO/DSS2) M5III, SRa (Mira-like) P = 141 days 0.7 M < M < 2 M Probable binary from Hipparcos astrometry 2 nd nearest AGB star (64 ± 4 pc, m V 5) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 2/14
3 Dimming event M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 3/14
4 Dimming event M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 3/14
5 VLT/NACO µm (March 2013) Kervella, Montargès et al. 2014, A&A, 564, A88 AO instrument, 12 narrow band filters in JHKL bands Lucky-imaging technique (5 000 exposures of 5 ms) Observation of a PSF for image deconvolution (β Col) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 4/14
6 VLT/NACO µm (March 2013) Kervella, Montargès et al. 2014, A&A, 564, A88 AO instrument, 12 narrow band filters in JHKL bands Lucky-imaging technique (5 000 exposures of 5 ms) Observation of a PSF for image deconvolution (β Col and α Lyn) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 4/14
7 Characteristics VLT/NACO observations VLT/SPHERE observations Open questions VLT/NACO (March 2013) - Deconvolved images M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 5/14
8 2.17 µm : VLT/NACO vs VLTI/AMBER M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 6/14
9 2.17 µm : VLT/NACO vs VLTI/AMBER M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 6/14
10 Characteristics VLT/NACO observations VLT/SPHERE observations Open questions VLT/NACO (March 2013) - Model Images M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 7/14
11 VLT/NACO (March 2013) - Composite image Results with NACO Dusty disk seen almost edge-on Modeling: photometry + shape M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 8/14
12 VLT/NACO (March 2013) - Composite image Results with NACO Dusty disk seen almost edge-on Modeling: photometry + shape Questions Why a disk? What are its effects on the stellar wind? What is the loop in the L band? M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 8/14
13 VLT/SPHERE (December 2014) VLT/SPHERE: ZIMPOL Extreme adaptive optics instrument Access to visible spectral domain 2 filters at the same time Q, U polarimetric measurements M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 9/14
14 VLT/SPHERE (December 2014) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 9/14
15 VLT/SPHERE (December 2014) - L2 Pup B M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 10/14
16 VLT/SPHERE (December 2014) - L2 Pup B Kervella, Montargès et al. 2015, A&A, 578, A77 M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 10/14
17 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
18 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
19 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
20 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
21 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
22 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
23 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
24 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
25 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
26 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
27 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
28 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
29 VLT/SPHERE (December 2014) - Polarimetric signatures (Kervella, Montargès et al. 2015, A&A, 578, A77) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 11/14
30 VLT/SPHERE - Radiative transfer modeling 3D dust distribution model: RADMC-3D code (Dullemond 2012) Dusty disk seen almost edge-on AGB stellar disk partly hidden M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 12/14
31 VLT/SPHERE - Radiative transfer modeling 3D dust distribution model: RADMC-3D code (Dullemond 2012) Dusty disk seen almost edge-on AGB stellar disk partly hidden Photometry and general morphology well reproduced M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 12/14
32 VLT/SPHERE - Radiative transfer modeling (photometry) Flux (W.m 2.µm) RADMC-3D model SPHERE Kurucz 3500K Kurucz with extinction MIDI NACO Observations SPHERE Observations Photometry pre Wavelength (µm) Dusty disk model R in = 6 AU Incl. = 82 MgFeSiO 4 + MgFeSi 2 O 3 M dust = M = 0.08 M M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 13/14
33 Open questions Formation of: - the plumes? - the streamers? Interaction AGB wind/dusty disk? Nature of companion? Dynamics? M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 14/14
34 Open questions Formation of: - the plumes? - the streamers? Interaction AGB wind/dusty disk? Nature of companion? Dynamics? (NACO L band + SPHERE R band) Thank you for your attention! M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 14/14
35 Backups M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 15/14
36 Polarization law 70% 60% Degree of linear polarization pl 50% 40% 30% 20% 10% pmax=0.58 pmax=0.42 0% Scattering angle Theta (degrees) M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 16/14
37 Altitude relatively to the plane of the sky M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 17/14
38 Mass loss collimation Stellar wind Dust disk plane mas AU M. Montargès - STEPS 2015 Garching The dusty disk and companion of L2 Puppis, a near AGB star, observed with VLT/SPHERE 18/14
THE SPHERE VIEW OF BETELGEUSE
Title : will be set by the publisher Editors : will be set by the publisher EAS Publications Series, Vol.?, 2013 THE SPHERE VIEW OF BETELGEUSE O. Chesneau 1, H.-M. Schmid 2, M. Carbillet 3, A. Chiavassa
Stuctural diversity resolving Herbig Ae/Be circumstellar Disks at AU using PDI
Stuctural diversity resolving Herbig Ae/Be circumstellar Disks at 10150 AU using PDI Henning Avenhaus Institute for Astronomy, ETH Zürich 2013 ROCKS! Conference, Hawaii Sascha Quanz, Hans Martin Schmid,
Stuctural diversity resolving Herbig Ae/Be circumstellar Disks at AU using PDI
Stuctural diversity resolving Herbig Ae/Be circumstellar Disks at 10150 AU using PDI Henning Avenhaus Institute for Astronomy, ETH Zürich 2013 ROCKS! Conference, Hawaii Sascha Quanz, Hans Martin Schmid,
About the angular diameter of red supergiant stars
Mass loss of evolved stars Betlegeuse/PIONIER Antares/PIONIER CE Tau/PIONIER Conclusion About the angular diameter of red supergiant stars Miguel Montargès (IRAM) VLTI Community Days ESO Garching - March
Near -IR interferometry:
Near -IR interferometry: spectrally dispersed JHK-band IOTA / GI2T interferograms, advantages of NIR, and aims Gerd Weigelt Max-Planck Institute for Radioastronomy, Bonn Plan Interferometry with spectrally
Exoplanets in the mid-ir with E-ELT & METIS
Exoplanets in the mid-ir with E-ELT & METIS Wolfgang Brandner (MPIA), Eric Pantin (CEA Saclay), Ralf Siebenmorgen (ESO), Sebastian Daemgen (MPIA/ESO), Kerstin Geißler (MPIA/ESO), Markus Janson (MPIA/Univ.
Recent VLTI results on stellar winds and perspectives with second generation instruments. Xavier Haubois
Recent VLTI results on stellar winds and perspectives with second generation instruments Xavier Haubois Outline - The VLTI and its instruments - Massive stars - HMXBs - AGBs - Planetary Nebulae - Perspectives
Spectropolarimetry: a tool for characterisation of exoplanets
Spectropolarimetry: a tool for characterisation of exoplanets Armagh. Observat ry March 31st, 2015 Polarisation I unpolarised partially polarised 100% polarised Polarisation II Image credit: http://www.tiffen.com/hi-res/polarizer-compare.jpg
Searching for extrasolar planets with SPHERE. Mesa Dino, Raffaele Gratton, Silvano Desidera, Riccardo Claudi (INAF OAPD)
Searching for extrasolar planets with SPHERE Mesa Dino, Raffaele Gratton, Silvano Desidera, Riccardo Claudi (INAF OAPD) The field of extrasolar planets today At the moment 2017 planets have been discovered.
Late-Type Stars. Liz Humphreys (ESO)
Late-Type Stars Liz Humphreys (ESO) Markus Wittkowski, Alain Baudry, Eric Blackman, Jason Grunhut, Susanne Hoefner, Franz Kerschbaum, Pierre Kervella, Mikako Matsuura, Iain Mcdonald, Claudia Paladini,
Deep fields around bright stars ( Galaxies around Stars )
Deep fields around bright stars ( Galaxies around Stars ) Scientific context: the morphological evolution of faint field galaxies Near-IR observations ground-based observations with AO: PUEO/CFHT deep
Exoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges
Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak
Synergies between E-ELT and space instrumentation for extrasolar planet science
Synergies between E-ELT and space instrumentation for extrasolar planet science Raffaele Gratton and Mariangela Bonavita INAF Osservatorio Astronomico di Padova - ITALY Main topics in exo-planetary science
G.Witzel Physics and Astronomy Department, University of California, Los Angeles, CA , USA
E-mail: shahzaman@ph1.uni-koeln.de A.Eckart E-mail: eckart@ph1.uni-koeln.de G.Witzel Physics and Astronomy Department, University of California, Los Angeles, CA 90095-1547, USA N. Sabha M. Zamaninasab
IR spectro-interferometry of cool evolved stars
IR spectro-interferometry of cool evolved stars Keiichi Ohnaka Max-Planck-Institut für Radioastronomie Infrared Interferometry Group 1) Mid-IR interferometry of Mira stars 2) Near-IR spectro-interferometry
Near-Infrared Imaging Observations of the Orion A-W Star Forming Region
Chin. J. Astron. Astrophys. Vol. 2 (2002), No. 3, 260 265 ( http: /www.chjaa.org or http: /chjaa.bao.ac.cn ) Chinese Journal of Astronomy and Astrophysics Near-Infrared Imaging Observations of the Orion
Exoplanets Direct imaging. Direct method of exoplanet detection. Direct imaging: observational challenges
Black body flux (in units 10-26 W m -2 Hz -1 ) of some Solar System bodies as seen from 10 pc. A putative hot Jupiter is also shown. The planets have two peaks in their spectra. The short-wavelength peak
Formation and Evolution of Planetary Systems
Formation and Evolution of Planetary Systems Meyer, Hillenbrand et al., Formation and Evolution of Planetary Systems (FEPS): First Results from a Spitzer Legacy Science Program ApJ S 154: 422 427 (2004).
ATMOSPHERES OF C-RICH AGB STARS OBSERVATIONS AND MODELS
ATMOSPHERES OF C-RICH AGB STARS OBSERVATIONS AND MODELS Gioia Rau University of Vienna - Institute for Astrophysics Blowing in the Wind, 8 August 2016 Collaborators: B. Aringer, K. Eriksson, M. A. T. Groenewegen,
arxiv:astro-ph/ v1 5 Nov 2004
Astronomy & Astrophysics manuscript no. hr4049 June 13, 2018 (DOI: will be inserted by hand later) VINCI-VLTI measurements of HR 4049: the physical size of the circumbinary envelope S. Antoniucci 1,2,3,
SPHERE GTO Program S. Desidera On behalf of SPHERE GTO team
SPHERE GTO Program S. Desidera On behalf of SPHERE GTO team Aims Provide an overview of the SPHERE GTO program to have a clear view of what is already on-going GTO targets (for the requested observing
arxiv:astro-ph/ v1 23 Oct 2002
Evolution of the symbiotic nova RX Puppis J. Mikołajewska, E. Brandi, L. Garcia, O. Ferrer, C. Quiroga and G.C. Anupama arxiv:astro-ph/0210505v1 23 Oct 2002 N. Copernicus Astronomical Center, Bartycka
FINITO: Three-Way Interferometric Fringe Sensor for VLTI
FINITO: Three-Way Interferometric Fringe Sensor for VLTI M. Gai 1, L. Corcione 1, M.G. Lattanzi 1, B. Bauvir 2, D. Bonino 1, D. Gardiol 1, A. Gennai 2, D. Loreggia 1, G. Massone 1, S. Menardi 2 1 INAF
Transitional disks and their host stars
Transitional disks and their host stars Nienke vander dermarel Marel Nienke van Leiden Observatory rd September 23 2011 The Netherlands August 13th 2013 (ING) Star and planet formation Class II => III:
From AGB Stars to Planetary Nebula. Cats Eye Planetary Nebula: HST
From AGB Stars to Planetary Nebula Cats Eye Planetary Nebula: HST AGB Stars NOAO H -> He in convective region Dredge Up Prialnik AGB stars pulsing Schwarzchild & Harm (1967) The 9th Cycle Schwarzchild
First Scientific Results from the VLT Interferometer*
First Scientific Results from the VLT Interferometer* Francesco Paresce, Roy Van Boekel, Serge Correia, Emmanuel Di Folco, Andreas Glindemann, Pierre Kervella, Andrea Richichi, Markus Schoeller, Massimo
ζ Pup: the merger of at least two massive stars?
ζ Pup: the merger of at least two massive stars? Dany Vanbeveren Astrophysical Institute, Vrije Universiteit Brussel and Leuven Engineering College, GroupT, Association KU Leuven Abstract. We first discuss
INTERFEROMETRIC OBSERVATIONS OF EVOLVED STARS
INTERFEROMETRIC OBSERVATIONS OF EVOLVED STARS Iva KAROVICOVA MPIA Heidelberg, Germany M. WITTKOWSKI ESO Garching, Germany D. A. BOBOLTZ Naval Observatory, USA E. FOSSAT Observatoire de la Côte d'azur,
AGB stars and their environment. Michel Guélin (Presenter: Ka Tat Wong) Institut de Radioastronomie Millimétrique (IRAM) Grenoble, France
AGB stars and their environment Michel Guélin (Presenter: Ka Tat Wong) Institut de Radioastronomie Millimétrique (IRAM) Grenoble, France 1. AGB stars and their winds: why, how? 2. New interferometric observations
E-ELT METIS * AND MATISSE: PROSPECTS FOR AGB-STARS
E-ELT METIS * AND MATISSE: PROSPECTS FOR AGB-STARS J. Hron 1, J. Blommaert 2, L. Decin 2, T. Lebzelter 1, C. Paladini 3,1, H. Van Winckel 2 and the METIS and MATISSE teams (1) Universitätssternwarte Wien,
M Giants (and their friends)
M Giants (and their friends) Gray & Corbally, Chapter 8 Eliot Halley Vrijmoet 2017 March 8 Image: ESO/ P. Kervella Outline History and significance of M giants Assessing temperatures Assessing luminosities
ORIENTATION EFFECTS IN BIPOLAR PLANETARY NEBULAE
The Astrophysical Journal, 675:380 388, 2008 March 1 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. ORIENTATION EFFECTS IN BIPOLAR PLANETARY NEBULAE Hugo E. Schwarz,
arxiv: v1 [astro-ph.sr] 9 Aug 2009
![arxiv: v1 [astro-ph.sr] 9 Aug 2009](/thumbs/74/69970859.jpg "arxiv: v1 [astro-ph.sr] 9 Aug 2009")
Astronomy & Astrophysics manuscript no. 11960 c ESO 2017 December 24, 2017 VLTI/MIDI observations of 7 classical Be stars A. Meilland 1, Ph. Stee 2, O. Chesneau 2, and C. Jones 3 arxiv:0908.1239v1 [astro-ph.sr]
Extrasolar Planet Science with High-Precision Astrometry Johannes Sahlmann
Extrasolar Planet Science with High-Precision Astrometry Johannes Sahlmann Geneva Observatory The First Years Of ESO, Garching, 4.9.212 high-precision astrometry is powerful yields complete information,
Gemini Planet Imager. Raphaël Galicher from presentations provided by James Graham and Marshall Perrin
Gemini Planet Imager from presentations provided by James Graham and Marshall Perrin Outline Ojectives The instrument Three examples of observations The GPI Exoplanet Survey 2 Objectives Radial velocity
The innermost circumstellar environment of massive young stellar objects revealed by infrared interferometry
The innermost circumstellar environment of massive young stellar objects revealed by infrared interferometry Thomas Preibisch, Stefan Kraus, Keiichi Ohnaka Max Planck Institute for Radio Astronomy, Bonn
Techniques for measuring astronomical distances generally come in two variates, absolute and relative.
Chapter 6 Distances 6.1 Preliminaries Techniques for measuring astronomical distances generally come in two variates, absolute and relative. Absolute distance measurements involve objects possibly unique
ASTR2050 Spring Please turn in your homework now! In this class we will discuss the Interstellar Medium:
ASTR2050 Spring 2005 Lecture 10am 29 March 2005 Please turn in your homework now! In this class we will discuss the Interstellar Medium: Introduction: Dust and Gas Extinction and Reddening Physics of Dust
Resolving the hot atmospheres of evolved stars with ALMA LBs. Wouter Vlemmings, Chalmers Univ. of Technology w. Theo Khouri, Eamon O Gorman et al.
Resolving the hot atmospheres of evolved stars with ALMA LBs Wouter Vlemmings, Chalmers Univ. of Technology w. Theo Khouri, Eamon O Gorman et al. AGB mass loss (before) dust formation Ballistic motions
Lecture 11: SDSS Sources at Other Wavelengths: From X rays to radio. Astr 598: Astronomy with SDSS
Astr 598: Astronomy with SDSS Spring Quarter 4, University of Washington, Željko Ivezić Lecture : SDSS Sources at Other Wavelengths: From X rays to radio Large Surveys at Many Wavelengths SDSS: UV-IR five-band
The binarity of young massive stars
School of Physics and Astronomy FACULTY OF MATHEMATICS AND PHYSICAL SCIENCES The binarity of young massive stars René Oudmaijer, Robert Pomohaci (Leeds, UK) Deborah Baines (Madrid, Spain) Willem-Jan de
Astronomy across the spectrum: telescopes and where we put them. Martha Haynes Discovering Dusty Galaxies July 7, 2016
Astronomy across the spectrum: telescopes and where we put them Martha Haynes Discovering Dusty Galaxies July 7, 2016 CCAT-prime: next generation telescope CCAT Site on C. Chajnantor Me, at 18,400 feet
Investigating the origin of stellar jets with SPHERE
Investigating the origin of stellar jets with SPHERE HH 30 - HST Linda Podio (INAF-Arcetri) & Simone Antoniucci (INAF-Rome) SPHERE Consortium SVT proposal (1 target): Dec 1-12 2014 P94 EGTO-Other Science
High Redshift Universe
High Redshift Universe Finding high z galaxies Lyman break galaxies (LBGs) Photometric redshifts Deep fields Starburst galaxies Extremely red objects (EROs) Sub-mm galaxies Lyman α systems Finding high
PLANETARY NEBULAE AND ALMA. Patrick Huggins, New York University
PLANETARY NEBULAE AND ALMA Patrick Huggins, New York University Abell 39 PNe: Overview Reminders evolution: AGB stars proto-pne PNe white dwarfs properties Problems and challenges current observational
Exploring the water and carbon monoxide shell around Betelgeuse with VLTI/AMBER
Exploring the water and carbon monoxide shell around Betelgeuse with VLTI/AMBER Miguel Montargès, Pierre Kervella, Guy Perrin, Keiichi Ohnaka To cite this version: Miguel Montargès, Pierre Kervella, Guy
Central supermassive black holes from SINFONI observations
Central supermassive black holes from SINFONI observations R.P Saglia, MPE with R.Bender, N.Nowak, P. Erwin, J. Thomas Gas and stars in Galaxies A Multi-Wavelength 3D Perspective Garching, 10th June 2008
arxiv: v1 [astro-ph.sr] 9 Oct 2018
![arxiv: v1 [astro-ph.sr] 9 Oct 2018](/thumbs/87/97204583.jpg "arxiv: v1 [astro-ph.sr] 9 Oct 2018")
Astronomy & Astrophysics manuscript no. Arxiv Version ESO 218 October 1, 218 High-resolution observations of gas and dust around Mira using ALMA and SPHERE/ZIMPOL T. Khouri 1, W. H. T. Vlemmings 1, H.
Searching for Binary Y dwarfs with the Gemini GeMS Multi-Conjugate Adaptive Optics System
Searching for Binary Y dwarfs with the Gemini GeMS Multi-Conjugate Adaptive Optics System Daniela Opitz 1,2, Chris Tinney 1,2 1 Exoplanetary Science Group, School of Physics, University of New South Wales,
GHOST. GIARPS High-resolution ObservationS of T Tauri Stars. S. Antoniucci (INAF- OAR)
JEts and Disks @Inaf GHOST GIARPS High-resolution ObservationS of T Tauri Stars S. Antoniucci (INAF- OAR) B. Nisini, T. Giannini (OAR), K. Biazzo, A. Frasca (OACt), J. M. Alcalà (OACn), D. Fedele, L. Podio,
Measuring Black Hole Masses in Nearby Galaxies with Laser Guide Star Adaptive Optics
Measuring Black Hole Masses in Nearby Galaxies with Laser Guide Star Adaptive Optics Claire Max Anne Medling Mark Ammons UC Santa Cruz Ric Davies Hauke Engel MPE-Garching Image of NGC 6240: Bush et al.
Galaxies. The majority of known galaxies fall into one of three major classes: spirals (78 %), ellipticals (18 %) and irregulars (4 %).
Galaxies Collection of stars, gas and dust bound together by their common gravitational pull. Galaxies range from 10,000 to 200,000 light-years in size. 1781 Charles Messier 1923 Edwin Hubble The distribution
Brown Dwarfs and Planets around Nearby Stars. A Coronagraphic Search for. B. R. Oppenheimer (AMNH) Morino,, H. Suto,, M. Ishii, M. K.
A Coronagraphic Search for Brown Dwarfs and Planets around Nearby Stars T. Nakajima, J.-I. Morino,, H. Suto,, M. Ishii, M. Tamura, N. Kaifu,, S. Miyama, H. Takami,, N. Takato, S. Oya, S. Hayashi, M. Hayashi
A high-contrast adaptiveoptics imaging search for brown dwarfs
http://en.wikipedia.org/wiki/file: Albert_Abraham_Michelson2.jpg A high-contrast adaptiveoptics imaging search for brown dwarfs http://nexsci.caltech.edu/sagan/ Katie Morzinski UC Santa Cruz/Center for
A powerful tool to uncover! hidden monsters? Daniel Asmus! ESO, Chile
A powerful tool to uncover hidden monsters? Daniel Asmus ESO, Chile Asmus et al. 2014 Only use those objects with: - reliable AGN classification, - no composites, - good S/N X-ray data - consistent intrinsic
The Mira variable S Ori: SiO maser shells related to the photosphere and dust shell at 3 epochs
The Mira variable S Ori: SiO maser shells related to the photosphere and dust shell at 3 epochs Program of coordinated interferometry of oxygen-rich evolved stars at near-infrared, mid-infrared, and radio
Identification of compact objects in X-ray/gamma-ray binaries and the exploration of long-period exoplanets by high-precision astrometry
X-ray binary Gaia Gaia-JASMINE Joint Meeting @NAOJ, 6-9 Dec. 2016 exoplanet ESA/ATG NAOJ Identification of compact objects in X-ray/gamma-ray binaries and the exploration of long-period exoplanets by high-precision
Supplemental Materials to An Imaging Survey for Extrasolar Planets around 54 Close, Young Stars with SDI at the VLT and MMT 1
Supplemental Materials to An Imaging Survey for Extrasolar Planets around 54 Close, Young Stars with SDI at the VLT and MMT 1 Beth A. Biller 1, Laird M. Close 1, Elena Masciadri 2, Eric Nielsen 1, Rainer
IRS SPECTRA OF SOLAR-TYPE STARS: A SEARCH FOR ASTEROID BELT ANALOGS
IRS SPECTRA OF SOLAR-TYPE STARS: A SEARCH FOR ASTEROID BELT ANALOGS Debris disks Around Stars In our Solar System, dust is generated by collisions between larger bodies in the asteroid and Kuiper belts,
How to calibrate interferometric data
National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology How to calibrate interferometric data Rachel Akeson 28 July 2006 Outline Calibration basics System
Exozodiacal discs with infrared interferometry
Exozodiacal discs with infrared interferometry First results and perspectives * (post-doc at LAOG, Grenoble) and E. Di Folco (Obs. Geneva), J.C. Augereau (LAOG), V. Coudé du Foresto (Obs. Paris), A. Mérand
Exoplanet Search Techniques: Overview. PHY 688, Lecture 28 April 3, 2009
Exoplanet Search Techniques: Overview PHY 688, Lecture 28 April 3, 2009 Course administration final presentations Outline see me for paper recommendations 2 3 weeks before talk see me with draft of presentation
Searching for Other Worlds
Searching for Other Worlds Lecture 32 1 In-Class Question What is the Greenhouse effect? a) Optical light from the Sun is reflected into space while infrared light passes through the atmosphere and heats
Point spread function reconstruction at W.M. Keck Observatory : progress and beyond
Point spread function reconstruction at W.M. Keck Observatory : progress and beyond Olivier Beltramo-Martin Aix-Marseille Univ., LAM, A*MIDEX, Extra November 9th, 217 - LAM Olivier Beltramo-Martin (LAM)
Introduction to exoplanetology
Introduction to exoplanetology Lesson #6: Direct exoplanet detection methods (1/2) Olivier Absil absil@astro.ulg.ac.be Outline I. Direct detection: why and how? II. High contrast imaging from the ground
Continuum and Line ALMA band 5: the supergiant VY CMa
Continuum and Line Polarisation @ ALMA band 5: the supergiant VY CMa Wouter Vlemmings, Chalmers Univ. of Technology w. Theo Khouri, Daniel Tafoya, Ivan Marti-Vidal, Liz Humphreys, Anita Richards, Eamon
Measuring stellar distances.
Measuring stellar distances This method can be used to measure distances up to 100pc Some new technology allows measuring distances up to 200pc using this method p= 1/d Stellar Parallax.htm This method
The Potential of Ground Based Telescopes. Jerry Nelson UC Santa Cruz 5 April 2002
The Potential of Ground Based Telescopes Jerry Nelson UC Santa Cruz 5 April 2002 Contents Present and Future Telescopes Looking through the atmosphere Adaptive optics Extragalactic astronomy Planet searches
Atmospheric Dynamics & Winds of AGB stars: A Theorist's View. Susanne Höfner Department of Physics and Astronomy Uppsala University
Atmospheric Dynamics & Winds of AGB stars: A Theorist's View Susanne Höfner Department of Physics and Astronomy Uppsala University Overview Dynamical atmospheres convection, pulsation, extended structures
AS750 Observational Astronomy
Lecture 9 0) Poisson! (quantum limitation) 1) Diffraction limit 2) Detection (aperture) limit a)simple case b)more realistic case 3) Atmosphere 2) Aperture limit (More realistic case) Aperture has m pixels
Effects of Massive Stars
Effects of Massive Stars Classical HII Regions Ultracompact HII Regions Stahler Palla: Sections 15.1, 15. HII Regions The salient characteristic of any massive star is its extreme energy output, much of
Lecture 12. November 20, 2018 Lab 6
Lecture 12 November 20, 2018 Lab 6 News Lab 4 Handed back next week (I hope). Lab 6 (Color-Magnitude Diagram) Observing completed; you have been assigned data if you were not able to observe. Due: instrumental
Monitoring Site Parameters for AO
Monitoring Site Parameters for AO Marc Sarazin, G. Lombardi, J. Navarrete, A. Tokovinin, R. Wilson ESO Garching, ESO Paranal CTIO La Serena, Durham University 1 Monitoring Site Parameters for AO ABSTRACT
The Binary System VV Cephei Eclipse Campaign 2017/2019 OHP-Meeting July 2017
The Binary System VV Cephei Eclipse Campaign 2017/2019 OHP-Meeting July 2017 Ernst Pollmann International Working Group Active Spectroscopy in Astronomy http://astrospectroscopy.de 3 One of the best known
Christophe Pinte. Multi-technique observations and modelling of protoplanetary disks. University of Exeter
Multi-technique observations and modelling of protoplanetary disks Christophe Pinte University of Exeter Christophe Pinte Multi-technique modelling 1/12 Collaborators F. Ménard, G. Duchêne, J.C. Augereau,
NIR Silicate features and Statistics from IRAS data
NIR Silicate features and Statistics from IRAS data Ranjan Gupta Inter University Center for Astronomy and Astrophysics Pune-411007, India NIR Silicate features and Statistics from IRAS data p.1/46 Abstract
Eric Lagadec for Olivier Chesneau
Observations of binaries (with focus on PNe and PPNe) Eric Lagadec for Olivier Chesneau (Observatoire de la Cote d Azur) Why galaxies care about AGB stars III Morphologies of AGB and post-agb envelopes
Analyzing Spiral Galaxies Observed in Near-Infrared
Analyzing Spiral Galaxies Observed in Near-Infrared Preben Grosbøl European Southern Observatory Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany Abstract A sample of 54 spiral galaxies was observed
protoplanetary transition disks
protoplanetary transition disks (Harvard-CfA) 1. disk evolution and planets why does disk dispersal matter? 40 AU orbit 2. transition disks definitions and observational signatures SMA 880 microns 3. resolved
, Th. Preibisch ', P. Stee 2, G. Weigelt ' Max-Planck-Institut f ur Radioastronomie, Auf dem H ugel 69, Bonn, Germany
Stars with the B[e] phenomenon ASP Conference Series, Vol. **VOLUME**, Michaela Kraus & Anatoly S. Miroshnichenko The vicinity of the galactic supergiant B [e] star CPD-7 7 from near- and mid-ir long baseline
Interstellar Medium and Star Birth
Interstellar Medium and Star Birth Interstellar dust Lagoon nebula: dust + gas Interstellar Dust Extinction and scattering responsible for localized patches of darkness (dark clouds), as well as widespread
Raven Eyes Elliptical Galaxies and Star Clusters. T. J. Davidge November 24, 2015
Raven Eyes Elliptical Galaxies and Star Clusters T. J. Davidge November 24, 2015 Why Maffei1 and the Glimpse Clusters? Targets were selected at low Galactic latitudes to maximize chances of finding a suitable
The Color-Magnitude Diagram for local stars from Hipparcos. Red Giant Branch (RGB) Red clump. Absolute Magnitude Main Sequence. White dwarfs.
The Color-Magnitude Diagram for local stars from Hipparcos Absolute Magnitude Main Sequence Red clump Red Giant Branch (RGB) White dwarfs Kovalevsky 1998 Color Lebreton 2001 The Hipparcos H-R Diagram of
Resolved Starburst Clusters Near & Far
Resolved Starburst Clusters Near & Far Andrea Stolte I. Physikalisches Institut Universität zu Köln E-ELT Science May 2009 ESO Garching 1 Resolved Starburst Clusters Near & Far 1. Outstanding questions
6. Interstellar Medium. Emission nebulae are diffuse patches of emission surrounding hot O and
6-1 6. Interstellar Medium 6.1 Nebulae Emission nebulae are diffuse patches of emission surrounding hot O and early B-type stars. Gas is ionized and heated by radiation from the parent stars. In size,
VLTI/AMBER studies of the atmospheric structure and fundamental parameters of red giant and supergiant stars
**Volume Title** ASP Conference Series, Vol. **Volume Number** **Author** c **Copyright Year** Astronomical Society of the Pacific VLTI/AMBER studies of the atmospheric structure and fundamental parameters
A Tale of Star and Planet Formation. Lynne Hillenbrand Caltech
A Tale of Star and Planet Formation Lynne Hillenbrand Caltech Vermeer s The Astronomer (1688) Mauna Kea (last week) photos by: Sarah Anderson and Bill Bates Context: Our Sun The Sun is a completely average
arxiv: v1 [astro-ph.sr] 13 Mar 2015
![arxiv: v1 [astro-ph.sr] 13 Mar 2015](/thumbs/74/69828802.jpg "arxiv: v1 [astro-ph.sr] 13 Mar 2015")
Astronomy & Astrophysics manuscript no. aa_acher_arxiv c ESO 2015 March 18, 2015 The evolved circumbinary disk of AC Her: a radiative transfer, interferometric and mineralogical study M. Hillen 1, B.L.
CHARA Collaboration Year-Eight Science Review. VLTI update. F. Delplancke
VLTI update F. Delplancke Summary Infrastructure Current instruments: MIDI, AMBER, PIONIER Under test & commissioning: PRIMA 2 nd generation instruments Long Range Plan Infrastructure Infrastructure 4
Gas Accretion & Outflows from Redshift z~1 Galaxies
Gas Accretion & Outflows from Redshift z~1 Galaxies David C. Koo Kate Rubin, Ben Weiner, Drew Phillips, Jason Prochaska, DEEP2, TKRS, & AEGIS Teams UCO/Lick Observatory, University of California, Santa
How to Understand Stars Chapter 17 How do stars differ? Is the Sun typical? Location in space. Gaia. How parallax relates to distance
How to Understand Stars Chapter 7 How do stars differ? Is the Sun typical? Image of Orion illustrates: The huge number of stars Colors Interstellar gas Location in space Two dimensions are easy measure
Subaru-Australian collaboration on Technologies for Habitable Planet Spectroscopy
Subaru-Australian collaboration on Technologies for Habitable Planet Spectroscopy Mike Ireland Plus many others: thanks to Barnaby Norris and Nemanja Jovanovic for slides. Thanks to Yosuke Minowa for keeping
A Multi-Wavelength Study of the Outburst of V1647 Orionis
A Multi-Wavelength Study of the 03 06 Outburst of V1647 Orionis Mario van den Ancker 1 Davide Fedele 1,2,3 Monika Petr-Gotzens 1 Piero Rafanelli 3 1 ESO 2 Max-Planck Institut für Astronomie, Heidelberg,
Mass-Loss Rates and Luminosities of Evolved Stars in the Magellanic Clouds
Mass-Loss Rates and Luminosities of Evolved Stars in the Magellanic Clouds Martin Groenewegen Royal Observatory of Belgium/Koninklijke Sterrenwacht van België, Brussels (martin.groenewegen@oma.be) Monte
Interferometric Observations of Supergiants: Direct Measures of the Very Largest Stars
Interferometric Observations of Supergiants: Direct Measures of the Very Largest Stars Gerard T. van Belle PRIMA Instrument Scientist Observatory April 7, 2008 Interferometric Observations of Supergiants:
Stefan Kraus 1,2 Gerd Weigelt 1 Karl-Heinz Hofmann 1 Fabien Malbet 3 Antonella Natta 4 Thomas Preibisch 5 Dieter Schertl 1 + AMBER consortium
From circumstellar disks to planetary systems workshop 2009 November 5 ESO, Garching Image: ESO/Calçada Stefan Kraus 1,2 Gerd Weigelt 1 Karl-Heinz Hofmann 1 Fabien Malbet 3 Antonella Natta 4 Thomas Preibisch
CHARA/NPOI 2013 Science & Technology Review MIRC Observations of the O-star Triple Sigma Orionis
MIRC Observations of the O-star Triple Sigma Orionis Gail Schaefer Doug Gies John Monnier Nils Turner New Title: Do NPOI and CHARA Orbits Agree?... stay tuned... Sigma Orionis Image credit: Peter Wienerroither
Imaging with Micado at the E-ELT. WORKSHOP: Imaging at the E-ELT
Imaging with Micado at the E-ELT Renato Falomo INAF Observatory of Padova, Italy WORKSHOP: Imaging at the E-ELT 29 May 2009, Garching Resolved stellar population in Virgo (high SB) Detailed View of high
The Ṁass- loss of Red Supergiants
The Ṁass- loss of Red Supergiants Dr. Donald F. Figer Director, Center for Detectors Speaker: Yuanhao (Harry) Zhang RIT 9/12/13 1 9/12/13 2 Outline IntroducJon MoJvaJon Objects Method Need for SOFIA/FORCAST
HD Transition Disk Herbig Ae/Be stars 2014
a b HD142527 Transition Disk Herbig Ae/Be stars 2014 HD142527 ALMA results by Sebastián Pérez Simon Casassus Valentin Christiaens Francois Ménard also with Gerrit van der Plas, Pablo Román, Christian Flores,