Pisa Evolution Models for low-mass stars (Dell'Omodarme+, 2012)

Computer Science

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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).

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