Hostname: page-component-8448b6f56d-cfpbc Total loading time: 0 Render date: 2024-04-16T17:09:44.107Z Has data issue: false hasContentIssue false
  • English
  • Français

SpS5 - II. Stellar and wind parameters

Published online by Cambridge University Press:  05 March 2015

F. Martins ,
M. Bergemann ,
J. M. Bestenlehner ,
P. A. Crowther ,
W. R. Hamann ,
F. Najarro ,
M. F. Nieva ,
N. Przybilla ,
J. Freimanis  and
W. Hou
...Show all authors
F. Martins
Affiliation:
LUPM, CNRS & Université Montpellier II, Place Eugène Batailon, F-34095, Montpellier, email: fabrice.martins@univ-montp2.fr
M. Bergemann
Affiliation:
Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str.1, D-85741 Garching, Germany
J. M. Bestenlehner
Affiliation:
Armagh Observatory, College Hill, Armagh BT61 9DG, United Kingdom
P. A. Crowther
Affiliation:
Dept of Physics and Astronomy, Univ. of Sheffield, Hounsfield Road, Sheffield, UK, S3 7RH
W. R. Hamann
Affiliation:
Lehrstuhl Astrophysik der Univ. Potsdam, Am Neuen Palais 10, 14469 Potsdam, Germany
F. Najarro
Affiliation:
Centro de Astrobiología, Ctra. Torrejón Ajalvir km 4, 28850 Torrejón de Ardoz, Spain
M. F. Nieva
Affiliation:
Dr. Karl Remeis-Observatory Bamberg & ECAP, University Erlangen-Nuremberg, Sternwartstr. 7, D-96049 Bamberg, Germany
N. Przybilla
Affiliation:
Dr. Karl Remeis-Observatory Bamberg & ECAP, University Erlangen-Nuremberg, Sternwartstr. 7, D-96049 Bamberg, Germany
J. Freimanis
Affiliation:
Ventspils International Radio Astronomy Centre, Ventspils University College, Inzenieru iela 101a, LV-3600 Ventspils, Latvia
W. Hou
Affiliation:
The National Astronomical observatories, Chinese Academy of Science
L. Kaper
Affiliation:
Astronomical Institute Anton Pannekoek, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The development of infrared observational facilities has revealed a number of massive stars in obscured environments throughout the Milky Way and beyond. The determination of their stellar and wind properties from infrared diagnostics is thus required to take full advantage of the wealth of observations available in the near and mid infrared. However, the task is challenging. This session addressed some of the problems encountered and showed the limitations and successes of infrared studies of massive stars.

Keywords

infrared: starsstars: early-typestars: late-typestars: fundamental parametersstars: mass lossstars: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 420 - 428
Copyright
Copyright © International Astronomical Union 2015 

References

Barniske, , et al. 2008, A&A 486, 971Google Scholar
Bergemann, , et al. 2012, ApJ 751, 156CrossRefGoogle Scholar
Bestenlehner, , et al. 2011, A&A 530, L14Google Scholar
Crowther, , et al. 2006, ApJ 636, 1033CrossRefGoogle Scholar
Dessart, , et al. 2000, MNRAS 315, 407CrossRefGoogle Scholar
Meynet, & Maeder, 2003, A&A 404, 975Google Scholar
Najarro, , et al. 2011, A&A 535, A32Google Scholar
Najarro, , et al. 2009, ApJ 691, 1816CrossRefGoogle Scholar
Najarro, , et al. 2006, ApJ 456, 659Google Scholar
Nieva, , et al. 2011, BSRSL 80, 175Google Scholar
Przybilla, , et al. 2009, in: Science with the VLT in the ELT Era, ed. Moorwood, A. (Springer, Netherlands)Google Scholar
Przybilla, & Butler, 2004, ApJ 609, 1181CrossRefGoogle Scholar
Repolust, , et al. 2005, A&A 440, 261Google Scholar