Helium ignition in rotating magnetized CO white dwarfs leading to fast and faint rather than classical Type Ia supernovae

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Table 1

Physical parameters of the initial white dwarf models.

M_WD,i	log (L_s,i/L_⊙)	T_c,i	ρ_c,i	R_WD,i	v_rot,i
M_⊙		10⁷ K	10⁶ g/cm³	R_⊙	km s^-1

0.54	−0.006	0.621	3.33	0.0141	10.0
0.54	−0.998	0.427	3.52	0.0133	10.3
0.54	−2.003	0.176	3.65	0.0126	10.6

0.82	−0.004	0.660	11.4	0.0105	17.1
0.82	−1.024	0.417	11.8	0.0101	9.5
0.82	−1.998	0.168	12.1	0.0098	9.4

1.00	−0.001	0.783	31.7	0.0083	9.4
1.00	−1.000	0.414	32.8	0.0080	9.5
1.00	−1.995	0.155	33.6	0.0078	9.3

1.10	−0.011	0.858	65.5	0.0070	7.4
1.10	−1.017	0.317	68.5	0.0068	7.3

Notes. Columns are: initial mass M_WD,i, initial surface luminosity L_s,i, initial core temperature T_c,i, initial core density ρ_c,i, initial radius R_WD,i and initial surface velocity v_rot,i.

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