2007/12/01 by Georges Meynet, Sylvia Ekstrom, Sylvia Ekström +5 · 7 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Feature (linguistics) #Rotation (mathematics) #Star (game theory) #Stars #Stellar evolution #Stellar rotation #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.1017/s1743921308020449
published in Proceedings of the International Astronomical Union 3(S250), 147-160 (Cambridge University Press) · 13 pages, 10 figures, IAU Symp. 250, Massive stars as Cosmic Engines, F. Bresolin, P.A. Crowther, J. Puls Eds
openalex publication_date 2007/12/01 · arxiv created 2008/02/20 · arxiv updated 2009/12/01 · openalex created_date 2020/03/13 · openalex updated_date 2026/08/05
Abstract New constraints on stellar models are provided by large surveys of massive stars, interferometric observations and asteroseismology. After a review of the main results so far obtained, we present new results from rotating models and discuss comparisons with observed features. We conclude that rotation is a key feature of massive star physics.