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: Mass limits for the different evolutionary scenarios (see text).
• Table 3: Lifetimes in Myr of WR stars of different initial masses and metallicities. The durations of various WR subphases are also indicated as well as theoretical predictions for various number ratios.