Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 $M_{\odot}$, and from $Z=0.0004$ to 0.03

Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C.

doi:10.1051/aas:2000126

Public

Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 $M_{\odot}$, and from $Z=0.0004$ to 0.03

Published in Astronomy & Astrophysics Supplement Series • Feb 1, 2000

Authors:

L. Girardi

A. Bressan

G. Bertelli

Abstract

We present a large grid of stellar evolutionary tracks, which are suitable to modelling star clusters and galaxies by means of population synthesis. The tracks are presented for the initial chemical compositions , , , , (solar composition), and . They are computed with updated opacities and equation...

Subject

Astrophysics

Physics

Schwarzschild radius

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