Populations of massive stars in galaxies, implications for the stellar evolution theory

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 10 figures, IAU Symposium 241, A. Vazdekis and R. Peletier eds., CUP

Scientific paper

10.1017/S174392130700734X

After a brief review of the observational evidences indicating how the populations of Be stars, red/blue supergiants, Wolf-Rayet stars vary as a function of metallicity, we discuss the implications of these observed trend for our understanding of the massive star evolution. We show how the inclusion of the effects of rotation in stellar models improves significantly the correspondence between theory and observation.

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