Pre-main sequence evolutionary tracks (Landin+, 2009)

Details Pre-main sequence evolutionary tracks (Landin+, 2009) Pre-main sequence evolutionary tracks (Landin+, 2009)

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34940209l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/494/209. Originally published in: 2009A&A...494..209L

Computer Science

Models: Evolutionary, Stars: Pre-Main Sequence

Scientific paper

These data present new pre-main sequence evolutionary tracks (including apsidal motion constants and gyration radii) for 0.09, 0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, 1.2, 1.4, 1.6, 1.8, 2.0, 2.3, 2.5, 2.8, 3.0, 3.3, 3.5 and 3.8 solar masses. The track was generated with a modified version of D'Antona & Mazzitelli's code (the ATON code) described in Ventura et al. (1998A&A...334..953V). We include the combined distortions effects of tidal and rotational forces in the ATON code and the results are presented in four tables for four sets of tracks: standard models (including no distortion effect), binary models (including only tidal distortions), rotating models (including only rotational distortions) and rotating binary models (including both tidal and rotational distortions). All models were computed with solar metallicity (Z=0.0175, Y=0.27) and alpha=1.5 (mixing length theory parameter).
(4 data files).

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