Scaled solar tracks and isochrones (Bertelli+, 2009)

Details Scaled solar tracks and isochrones (Bertelli+, 2009) Scaled solar tracks and isochrones (Bertelli+, 2009)

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35080355b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/508/355. Originally published in: 2009A&A...508..355B

Computer Science

Models: Evolutionary, Magnitudes, Abundances

Scientific paper

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;.
(6 data files).

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