The advanced evolution of massive stars - I. New reaction rates for carbon and oxygen nuclear reactions

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Table 3.

Core-burning lifetimes (in years) for rotating and non-rotating stars of 15, 17, and 20 M_⊙ as a function of the adopted nuclear reaction rates.

C-burning
Model	V_ini/V_crit	CF88	HIN(RES)	TDHF

15 M_⊙	0	4024	4014	5426
	0.4	3014	2809	3759
17 M_⊙	0	2360	2372	3092
	0.4	1873	1651	2134
20 M_⊙	0	1059	1042	1418
	0.4	795	830	1070

Ne-burning

Model	V_ini/V_crit	CF88	HIN(RES)	TDHF

15 M_⊙	0	3.71	2.78	2.26
	0.4	2.26	2.41	1.51
17 M_⊙	0	3.2	5.82	2.75
	0.4	0.52	0.49	0.50
20 M_⊙	0	0.65	0.94	0.25
	0.4	0.75	0.32	1.30

O-burning

Model	V_ini/V_crit	CF88	HIN(RES)	TDHF

15 M_⊙	0	1.78	0.68	1.16
	0.4	1.04	0.59	1.20
17 M_⊙	0	0.80	0.70	0.73
	0.4	0.52	0.42	0.63
20 M_⊙	0	0.49	0.26	0.55
	0.4	0.45	0.18	0.37

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