Pre-main sequence evolutionary tracks (Landin+, 2010)

Computer Science

Scientific paper

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Models: Evolutionary, Stars: Pre-Main Sequence

Scientific paper

These data present pre-main sequence evolutionary tracks, including local and global convective turnover times and Rossby numbers, for 0.6, 0.7, 0.8, 0.9, 1.0, 1.1 and 1.2 solar masses. The tracks were generated with a modified version of D'Antona & Mazzitelli's code (the ATON code, Ventura et al., 1998A&A...334..953V) which take into account stellar rotation (Mendes et al., 1999A&A...341..174M). All models were computed with solar metallicity (Z=0.0175, Y=0.27) and alpha=1.5 (mixing length theory parameter).
(1 data file).

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