Evolutionary tracks and Isochrones in the Johnson-Cousins UBVRIJHK system for the compositions: Z=0.0001 (Y=0.23, 0.26, 0.30, 0.40) Z=0.0004 (Y=0.23, 0.26, 0.30, 0.40) Z=0.001 (Y=0.23, 0.26, 0.30, 0.40) Z=0.002 (Y=0.23, 0.26, 0.30, 0.40) Z=0.004 (Y=0.23, 0.26, 0.30, 0.40) Z=0.008 (Y=0.23, 0.26, 0.30, 0.34, 0.40) Z=0.017 (Y=0.23, 0.26, 0.30, 0.34, 0.40) Z=0.040 (Y= 0.26, 0.30, 0.34, 0.40, 0.46) Z=0.070 (Y= 0.30, 0.34, 0.40, 0.46) The evolutionary tracks include those presented in Paper I (Bertelli et al. 2008A&A...484..815B); the masses of the models cover the range 0.6 to 20M&sun;.
Scaled solar tracks and isochrones (Bertelli+, 2009)
MARIGO, PAOLA
2010
Abstract
Evolutionary tracks and Isochrones in the Johnson-Cousins UBVRIJHK system for the compositions: Z=0.0001 (Y=0.23, 0.26, 0.30, 0.40) Z=0.0004 (Y=0.23, 0.26, 0.30, 0.40) Z=0.001 (Y=0.23, 0.26, 0.30, 0.40) Z=0.002 (Y=0.23, 0.26, 0.30, 0.40) Z=0.004 (Y=0.23, 0.26, 0.30, 0.40) Z=0.008 (Y=0.23, 0.26, 0.30, 0.34, 0.40) Z=0.017 (Y=0.23, 0.26, 0.30, 0.34, 0.40) Z=0.040 (Y= 0.26, 0.30, 0.34, 0.40, 0.46) Z=0.070 (Y= 0.30, 0.34, 0.40, 0.46) The evolutionary tracks include those presented in Paper I (Bertelli et al. 2008A&A...484..815B); the masses of the models cover the range 0.6 to 20M&sun;.
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