Volume 366, Number 2, February I 2001
|Page(s)||538 - 546|
|Section||Interstellar and circumstellar matter|
|Published online||15 February 2001|
Database of Geneva stellar evolution tracks and isochrones for (UBV)(RI) JHKLL'M, HST-WFPC2, Geneva and Washington photometric systems*
Observatório Astronómico da Universidade de Coimbra, Santa Clara, 3040 Coimbra, Portugal
2 Astronomisches Institut der Universität Basel, Venusstr. 7, 4102 Binningen, Switzerland
3 Observatoire Midi-Pyrénées, Laboratoire d'Astrophysique, UMR 5572, 14 avenue E. Belin, 31400 Toulouse, France
Corresponding author: D. Schaerer, email@example.com
Accepted: 3 November 2000
We have used an updated version of the empirically and semi-empirically calibrated BaSeL library of synthetic stellar spectra of Lejeune et al.([CITE], [CITE]) and Westera et al.([CITE]) to calculate synthetic photometry in the (UBV) J (RI) C JHKLL ′ M, HST-WFPC2, Geneva, and Washington systems for the entire set of non-rotating Geneva stellar evolution models covering masses from 0.4-0.8 to 120-150 and metallicities (1/50 ) to 0.1 (5 ). The results are provided in a database which includes all individual stellar tracks and the corresponding isochrones covering ages from 103 yr to 16-20 Gyr in time steps of 0.05 dex. The database also includes a new grid of stellar tracks of very metal-poor stars () from calculated with the Geneva stellar evolution code.
Key words: stars: general / stars: evolution / stars: Hertzsprung-Russell diagram / stars: fundamental parameters
© ESO, 2001
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