  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.
