Recent Progress in Modeling Stellar Atmospheres

Details Recent Progress in Modeling Stellar Atmospheres Recent Progress in Modeling Stellar Atmospheres

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nqsa.conf..211h&link_type=abstract

New Quests in Stellar Astrophysics. II. Ultraviolet Properties of Evolved Stellar Populations, Proceedings of the International

Astronomy and Astrophysics

Astrophysics

Scientific paper

We briefly review recent progress in modeling stellar atmospheres. We first summarize various levels of approximations being used in constructing the models, and present a brief overview of existing model atmosphere codes. We then concentrate on a description of our universal computer program Tlusty, and our recent grids of NLTE metal line blanketed model photospheres of O-stars - OSTAR2002 - and early B-stars - BSTAR2006.

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