1994/10/14 by D. Schaerer, Schaerer, D., A. de Koter +4
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #Astrophysics and Star Formation Studies #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9410046
JD16 IAU General Assembly, "Astrophysical Applications of Powerful New Atomic Databases", ASP Conf. Series, Eds. S. Adelman, W.L. Wiese, 5 pages, uuencoded postscript with 2 figures, DS-10-94
arxiv created 1994/10/14 · openalex publication_date 1994/10/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/24 · openalex updated_date 2026/07/28
In this paper we present Complete Stellar models (CoStar) for massive stars,\nwhich treat the stellar interior and atmosphere, including its wind. Particular\nemphasis is given to Wolf-Rayet stars. We address the question of the effective\ntemperatures of WNE and WC stars. Our first results show a satisfactory\nagreement between the CoStar models and the simple temperature correction\nmethod applied by Schaller et al. (1992). An analyses of the subphotospheric\nstructure of the WR star models shows the importance of metal opacity. This may\nbe essential for understanding the driving mechanism of Wolf-Rayet winds.\n