Disk-locking PMS evolutionary tracks

Rotational evolution in young stars is described by pre-main sequence evolutionary tracks including non-gray boundary conditions, rotation, conservation of angular momentum, and...年轻恒星的自转演化可通过包含非灰体边界条件（non-gray boundary conditions）、自转效应与角动量守恒等物理要素的前主序星（pre-main sequence）演化轨迹进行描述。