著者: C. Georgy, Sylvia Ekström, P. Eggenberger, G. Meynet, L. Haemmerlé, A. Maeder, A. Granada, J. H. Groh, Raphaël Hirschi, N. Mowlavï, Norhasliza Yusof, C. Charbonnel, T. Decressin, F. Barblan - Astronomy and Astrophysics 2013 被引用: 379
Aims. We study the impact of a subsolar metallicity on various properties of non-rotating and rotating stars, such as surface velocities and abundances, lifetimes, evolutionary tracks, and evolutionary scenarios.
