SpS5 - II. Stellar and wind parameters

Fabrice Martins; M. Bergemann; J.M. Bestenlehner; P.A. Crowther; W.R. Hamann; F. Najarro; M.F. Nieva; N. Przybilla; J. Freimanis; W. Hou; L. Kaper; C.-D. Lee

doi:10.1017/S1743921314011788

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SpS5 - II. Stellar and wind parameters

Fabrice Martins, M. Bergemann, J.M. Bestenlehner, P.A. Crowther, W.R. Hamann, F. Najarro, M.F. Nieva, N. Przybilla, J. Freimanis, W. Hou, …

IAU Symp, Vol.16, pp.420-428

28th General Assembly of the International Astronomical Union (IAU) (Beijing, China, 20/08/2012–31/08/2012)

2015

DOI: https://doi.org/10.1017/S1743921314011788

Résumé

infrared: stars

stars: early-type

stars: late-type

stars: fundamental parameters

stars: mass loss

stars: abundances

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.

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Détails

Titre: SpS5 - II. Stellar and wind parameters
Créateurs - sans rôle: Fabrice Martins - Université de Montpellier, Laboratoire Univers et Particules de Montpellier - LUPM
M. Bergemann - Max Planck Institute for Astrophysics
J.M. Bestenlehner - Armagh Observatory & Planetarium
P.A. Crowther - University of Sheffield
W.R. Hamann
F. Najarro - Centro de Astrobiología
M.F. Nieva - University of Bamberg
N. Przybilla - University of Bamberg
J. Freimanis - Ventspils University of Applied Sciences
W. Hou - National Astronomical Observatories
L. Kaper - University of Amsterdam
C.-D. Lee
Détails de publication: IAU Symp, Vol.16, pp.420-428
Colloque: 28th General Assembly of the International Astronomical Union (IAU) (Beijing, China, 20/08/2012–31/08/2012)
Identifiants: 9943520309311
Unité académique: Laboratoire Univers et Particules de Montpellier - LUPM
Langue: English
Type de ressource: Conference proceeding
Champs locaux: hal-02016897