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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

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Girardi, L., Bressan, A., Bertelli, G., Chiosi, C.·2000·Astronomy and Astrophysics Supplement Series

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 of state, and a moderate amount of convective overshoot. The range of initial masses goes from to , and the evolutionary phases extend from the zero age main sequence (ZAMS) till either the thermally pulsing AGB regime or carbon ignition. We also present an additional set of models with solar composition, computed using the classical Schwarzschild criterion for convective boundaries. From all these tracks, we derive the theoretical isochrones in the Johnson-Cousins UBVRIJHK broad-band photometric system.

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Metadata

Authors
Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C.
Venue
Astronomy and Astrophysics Supplement Series
Publisher
EDP Sciences
Published
2000-02
Volume
141
Issue
3
Pages
371-383
ISSN
  • 0365-0138 (ISSN-L)
  • 1286-4846
OpenAlex
W2134770831
Cited by
2,553
References
0
FWCI
76.08
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: 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. https://app.cochat.ai/papers/10.1051/aas:2000126
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Girardi, L., Bressan, A., Bertelli, G., & Chiosi, C. (2000). 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. Astronomy and Astrophysics Supplement Series. https://doi.org/10.1051/aas%3A2000126

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