Journal
ASTRONOMY & ASTROPHYSICS
Volume 366, Issue 2, Pages 538-546Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20000214
Keywords
stars : general; stars : evolution; stars : Hertzsprung-Russell diagram; stars : fundamental parameters
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We have used an updated version of the empirically and semi-empirically calibrated BaSeL library of synthetic stellar spectra of Lejeune et al. (1997, 1998) and Westera ct al. (1911'3) 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 front 0.4-0.8 to 120 150 M., and metallicities Z = 0.0004 (1/50 Z.) to 0.1 (5 Z.) The results are provided in a database which includes all individual stellar tracks and the corresponding isochrones covering ages from 10(3) yr to 16-20 Gyr in time steps of Delta log t = 0.05 dex. The database also includes a new grid of stellar tracks of very metal-poor stars (Z = 0.0004) from 0.8-150 M. calculated with the Geneva stellar evolution code.
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