Table 1: Parameters of the calculated models, a and b are parameters used in Eq. (4) with values of gravity darkening $\beta$ according to Claret (1998). Note that for all models profiles with $\beta = 0.0, 0.08$ and 0.25 were analyzed.
Model $T_{\rm eff}^{\rm Pole}$ $M/M_\odot$ $\beta$ a b

B0 30 000 17.5 0.25 .740E-4 -.345E-6

A0 10 000 2.4 0.25 .190E-3 -.136E-5

F0 7000 1.6 0.08 .172E-3 -.993E-6

G0 5700 1.0 0.08 .184E-3 -.116E-5

**Table 1:** Parameters of the calculated models, a and b are parameters used in Eq. (4) with values of gravity darkening $\beta$ according to Claret (1998). Note that for all models profiles with $\beta = 0.0, 0.08$ and 0.25 were analyzed.
Model	$T_{\rm eff}^{\rm Pole}$	$M/M_\odot$	$\beta$	a	b
B0	30 000	17.5	0.25	.740E-4	-.345E-6
A0	10 000	2.4	0.25	.190E-3	-.136E-5
F0	7000	1.6	0.08	.172E-3	-.993E-6
G0	5700	1.0	0.08	.184E-3	-.116E-5

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