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.
Mode P (day) $S_{\rm c}$ (Gauss^-2) $B_{\rm pol}$ (kG)

g₂₀¹ 1.497 $2.278\times 10^{-6}$ 111

g₁₅¹ 1.159 $3.765\times 10^{-7}$ 274

g₁₀¹ 0.789 $2.321\times 10^{-8}$ 1102

**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.
Mode	P (day)	$S_{\rm c}$ (Gauss^-2)	$B_{\rm pol}$ (kG)
g₂₀¹	1.497	$2.278\times 10^{-6}$	111
g₁₅¹	1.159	$3.765\times 10^{-7}$	274
g₁₀¹	0.789	$2.321\times 10^{-8}$	1102

Source LaTeX | All tables | In the text

	1 Introduction
	2 Magnetic frequency splitting of g modes
	3 Model
	4 Discussion
	References