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.
l=1 l=2

n $\nu$ ( $\mu$ Hz) P (d) n $\nu$ ( $\mu$ Hz) P (d)

23 6.683 1.732 40 6.761 1.712

20 7.728 1.498 35 7.730 1.497

15 9.983 1.159 30 9.035 1.281

10 14.68 0.788 25 10.86 1.066

5 29.31 0.395 10 25.15 0.460

**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.
	l=1		l=2
n	$\nu$ ( $\mu$ Hz)	P (d)	n	$\nu$ ( $\mu$ Hz)	P (d)
23	6.683	1.732	40	6.761	1.712
20	7.728	1.498	35	7.730	1.497
15	9.983	1.159	30	9.035	1.281
10	14.68	0.788	25	10.86	1.066
5	29.31	0.395	10	25.15	0.460

Source LaTeX | All tables | In the text

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