All Tables

Table 1: Properties of the computed models. The first column denotes the sequence number, where "NR'', "R'' and "RT'' denote the non-rotating models and rotating models with $f_{\rm c} = 1/30$ and 1/3 respectively. The second column gives the accretion rate in units of 10^-7 ${M}_{\odot }/\rm {yr}$ . The third column denotes the factor $f_{\rm c}$ for the chemical mixing efficiency in rotating models. Columns 4-7 give mass, central density, central temperature and $\ensuremath {E_{\rm rot}/\vert E_{\rm grav}\vert}$ of the last computed model of each evolutionary sequence. The eighth column gives the amount of accreted material until the onset of the helium shell instability. The column with $L_{\rm Edd}$ indicates whether the last computed model reached the Eddington limit or not. The last column gives the total number of the computed models for each sequence.