Zero-metallicity Stars I. Evolution at constant mass
We present extensive evolutionary models of stars with initial zero-metallicity, covering a large range of initial masses (i.e. 0.7 M⊙ ≤ M ≤ 100 M⊙). Calculations are carried out at constant mass, with updated input physics, and applying an oversh
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
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