Table 1: Some parameters of the considered model of stellar perturbations.

i	Type	M*i		N*i
1	B0	13.2	1 973 000	418
2	A0	2.4	803 000	343
3	A5	1.86	691 000	434
4	F0	1.55	568 000	1168
5	F5	1.32	482 000	450
6	G0	1.12	416 000	909
7	G5	0.98	389 000	1228
8	K0	0.82	384 000	1177
9	K5	0.68	311 000	1924
10	M0	0.52	285 000	2464
11	M5	0.27	204 000	6249
12	WD	0.6	242 000	983
13	gs.	2.2	580 000	503