All Tables

Table 1: Initial properties and lifetimes of central burning stages of solar metallicity models. Also given are the total mass and the different core masses at the end of central silicon burning as well as at the last time step of our calculations. These last models correspond approximatively to the end of the first shell silicon burning for non-rotating models and slightly later then central silicon burning for rotating ones. All masses are in solar mass units. Lifetimes are in years with exponent in brackets (2.14 $(-2)=2.14\times 10^{-2}$ ). Velocities are in km s^-1.
Table 2: Same as Table 1 for the 12 $M_{\odot }$ models. The non-rotating model starts Ne-burning off-centre and the burning never reaches the centre. The unburnt Ne-O core is given by $M_{\rm {Ne-O}}$ .
Table 3: Lifetimes of central burning stages of solar metallicity models. Lifetimes are in years with exponent in brackets (2.14 $(-2)=2.14\times 10^{-2}$ ).
Table 4: Final core masses at the pre-supernova stage for different models of non-rotating stars at solar metallicity.
Table 5: Final core masses at the pre-supernova stage for different models of rotating stars at solar metallicity. Note that we use $M_{\rm {Si}}$ at the end of central Si-burning for the value of $M_{\rm {Fe}}$ as discussed in the text.