Pre-Main Sequence Evolutions of Solar Abundance Lowmass Stars
Astrophysics
2016-07-20 v1
Abstract
We present the Pre-Main-Sequence (PMS) evolutionary tracks of stars with 0.0065~5.0Ms. The models were evolved from the PMS stellar birthline to the onset of hydrogen burning in the core. The convective turnover timescales which enables an observational test of theoretical model, particulary in the stellar dynamic activity, are also calculated. All models have Sun-like metal abundances, typically considered as the stars in the Galactic disk and the star formation region of Population I star. The convection phenomenon is treated by the usual mixing length approximation. All evolutionary tracks are available upon request.
Keywords
Cite
@article{arxiv.astro-ph/0702301,
title = {Pre-Main Sequence Evolutions of Solar Abundance Lowmass Stars},
author = {Youn Kil Jung and Yong-Cheol Kim},
journal= {arXiv preprint arXiv:astro-ph/0702301},
year = {2016}
}
Comments
30pages, 2figures