First evidence of inertial modes in γ Doradus stars: The core rotation revealed

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Table 3.

Characteristics of the resonances for zonal dipolar modes for the three models 1z, 2m, 3t given in Table 2 (radial order n, frequency of the mixed gravito-inertial – pure inertial mode ν_in, and corresponding spin parameter s) and for three uniform rotation frequencies 15, 19 and 23 μHz.

ν_rot		1z	2m	3t
	n	−43	−40	−45
15 μHz	ν_in (μHz)	13.30	13.89	13.93
	s	2.256	2.160	2.153

	n	−34	−32	−35
19 μHz	ν_in (μHz)	16.81	17.52	17.72
	s	2.261	2.169	2.145

	n	−29	−26	−29
23 μHz	ν_in (μHz)	20.04	21.29	21.15
	s	2.296	2.161	2.149

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