- 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.