Database of Geneva stellar evolution tracks and isochrones for (UBV)J(RI)C JHKLL′M, HST-WFPC2, Geneva and Washington photometric systems

被引:494
作者
Lejeune, T
Schaerer, D
机构
[1] Observ Midi Pyrenees, Astrophys Lab, UMR 5572, F-31400 Toulouse, France
[2] Univ Coimbra, Astron Observ, P-3040 Coimbra, Portugal
[3] Univ Basel, Inst Astron, CH-4102 Binningen, Switzerland
关键词
stars : general; stars : evolution; stars : Hertzsprung-Russell diagram; stars : fundamental parameters;
D O I
10.1051/0004-6361:20000214
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:538 / 546
页数:9
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