Impact of convective overshooting on the single-degenerate model of Type Ia supernovae

Open Access

Table 3.

SN Ia birth rate for δ_ov = 0.50.

M_WD/M_⊙	△log₁₀a	M_A/M_⊙	M_B/M_⊙	△q	ν/yr⁻¹	$\bar{ν} / {yr}^{- 1}$ $\bar{\nu}/\mathrm{yr}^{-1}$
0.675–0.7	0.07	2.83	3.20	0.0814	0.00003	0.00005
0.675–0.7	0.13	2.83	3.20	0.1167	0.00007

0.7–0.75	0.13	3.20	3.86	0.1396	0.00011	0.00040
0.7–0.75	0.60	3.20	3.86	0.1968	0.00068

0.75–0.8	0.60	3.86	4.48	0.1449	0.00030	0.00033
0.75–0.8	0.61	3.86	4.48	0.1708	0.00036

0.8–0.9	0.61	4.48	5.60	0.1744	0.00043	0.00085
0.8–0.9	0.91	4.48	5.60	0.3486	0.00127

0.9–1.0	0.91	5.60	6.63	0.2642	0.00054	0.00063
0.9–1.0	1.00	5.60	6.63	0.3178	0.00071

1.0–1.1	1.00	6.63	7.58	0.2607	0.00037	0.00043
1.0–1.1	1.07	6.63	7.58	0.3211	0.00050

1.1–1.2	1.07	7.58	8.48	0.2758	0.00030	0.00034
1.1–1.2	1.19	7.58	8.48	0.3286	0.00039

Notes. Same as Table 1 but for δ_ov = 0.50.

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