All Tables

• Table 1: Properties of the stellar models at the end of the H-burning phase and at the end of the He-burning phase. The masses are in solar mass, the velocities in km s^-1, the lifetimes in million years and the abundances in mass fraction.
• Table 2: Lifetimes of Wolf-Rayet star from various initial masses and velocities and predictions for different number ratios (see text). The velocities are in km s^-1 and the lifetimes in Myr.