Probing the shape of the mixing profile and of the thermal structure at the convective core boundary through asteroseismology

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Table 4.

Same as Table 2, but for the differences between the diffusive Gumbel and convective Gumbel prescriptions.

X_c	SPB			β Cep g modes			β Cep p modes

	4 yr	1 yr	90 d	4 yr	1 yr	90 d	4 yr	1 yr	90 d
0.7	72	56	16	100	70	40	100	100	100
0.6	100	66	22	80	30	10	100	100	100
0.5	100	74	30	100	20	10	100	100	100
0.4	100	100	38	90	40	20	100	100	100
0.3	100	100	42	100	50	10	100	100	100
0.2	100	100	48	90	60	20	100	100	100
0.1	100	100	52	90	80	10	100	100	100

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