We present new evolutionary models for zero-metallicity stars, covering a large range of initial masses (from 0.8 to 100 M_sun). Models are computed with overshooting from stellar cores and convective envelopes, and assuming mass-loss from the most massive stars. We discuss the main evolutionary features of these stars, and provide estimates of the amount of newly-synthesized elements dredged-up to the stellar surface, and possibly lost by stellar winds from the most massive stars. Full details of these models will be given in Marigo et al. (2000, in preparation).
CITATION STYLE
Marigo, P., Chiosi, C., Girardi, L., & Sarrubbi, T. (2006). Evolutionary Models of Zero Metallicity Stars. In The First Stars (pp. 119–120). Springer-Verlag. https://doi.org/10.1007/10719504_19
Mendeley helps you to discover research relevant for your work.