Evolution of long-lived globular cluster stars - IV. Initial helium content and white-dwarf properties

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Table 3

M_ini and M_WD of stars with an age of 9, 12 and 13 Gyr at the end of the central He-burning phase at [Fe/H] = –1.75.


Y _ini	13 Gyr		12 Gyr		9 Gyr


	M _ini	M _WD	M _ini	M _WD	M _ini	M _WD


0.248	0.82	0.58	0.84	0.60	0.91	0.68
0.270	0.79	0.56	0.81	0.59	0.88	0.65
0.280	0.78	0.55	0.79	0.57	0.86	0.65
0.300	0.75	0.52	0.77	0.55	0.83	0.63
0.400	0.63	0.47	0.64	0.47	0.70	0.50
0.600	0.41	0.35	0.42	0.36	0.45	0.39

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