All Tables

Table 1: Frequency and periods for g modes of different radial orders and degree l=1, for a 4 $M_\odot$ star with an age of 94 Myr.
Table 2: Splitting constant ( $S_{\rm c}$ ) and value of the polar field ( $B_{\rm pol}$ ), at the edge of the convective core for l=1 g modes that would produce a frequency splitting of $1\%$ , for a 4 $M_\odot$ star with an age of 94 Myr.
Table 3: Splitting coefficient ( $S_{\rm c}$ ) and value of the polar field ( $B_{\rm pol})$ , at the edge of the convective core for l=2 g modes corresponding to different transitions that would produce a frequency splitting of $1\%$ , for a 4 $M_\odot$ star with an age of 94 Myr.