All Tables

Table 1: Essential input parameter ranges covered by our collection of subsolar metallicity models.
Table 2: Variation of the carbon overabundance $\epsilon _{\rm C/O}$ for otherwise fixed parameters.
Table 3: Mass-loss rates of SMC, LMC, and solar wind models with identical input parameters; $\epsilon _{\rm C/O} = 1.8$ , $\Delta v = 5$ km s^-1, P = 500 d at 8000 $L_\odot$ , 600 d at 10 000 $L_\odot$ , and 700 d at 12 000 $L_\odot$ . Mass loss averages are over time interval 70-150 periods, or (1) 70-90, (2) 70-210.
Table 4: Stellar evolution grids: final masses and ages.