Computer Science
Scientific paper
Mar 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..35409026d&link_type=abstract
VizieR On-line Data Catalog: J/A+A/540/A26. Originally published in: 2012A&A...540A..26D
Computer Science
Stars: Horizontal Branch, Models: Evolutionary, Isochrones, Abundances, Stars: Ages, Stars: Masses
Scientific paper
Evolutionary tracks and Isochrones in the log L vs log Te plane, for the following chemical compositions:
Z Y Y Y Y Y Y 0.0001 0.249 0.250 0.270 0.330 0.380 0.420 0.0002 0.249 0.250 0.270 0.330 0.380 0.420 0.0003 0.249 0.250 0.270 0.330 0.380 0.420 0.0004 0.249 0.250 0.270 0.330 0.380 0.420 0.0005 0.250 0.250 0.270 0.330 0.380 0.420 0.0006 0.250 0.250 0.270 0.330 0.380 0.420 0.0007 0.250 0.250 0.270 0.330 0.380 0.420 0.0008 0.250 0.250 0.270 0.330 0.380 0.420 0.0009 0.250 0.250 0.270 0.330 0.380 0.420 0.0010 0.250 0.250 0.270 0.330 0.380 0.420 0.0020 0.252 0.250 0.270 0.330 0.380 0.420 0.0030 0.254 0.250 0.270 0.330 0.380 0.420 0.0040 0.256 0.250 0.270 0.330 0.380 0.420 0.0050 0.258 0.250 0.270 0.330 0.380 0.420 0.0060 0.260 0.250 0.270 0.330 0.380 0.420 0.0070 0.262 0.250 0.270 0.330 0.380 0.420 0.0080 0.264 0.250 0.270 0.330 0.380 0.420 0.0090 0.266 0.250 0.270 0.330 0.380 0.420 0.0100 0.268 0.250 0.270 0.330 0.380 0.420
Each model is calculated with three different values of the mixing length parameter alpha=1.70, 1.80, 1.90 and two different alpha-enhancement [alpha/Fe]=0.0, 0.3.
(11 data files).
Degl'Innocenti Scilla
Dell'Omodarme Matteo
Prada Moroni Pier Giorgio
Valle Glauco
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