Table 1
Main-sequence companion star models.
Model1 | Mwd | Mc,i | Mc,f | Pf | af | af/R2 | Mstripped | vkick | SNe Ia2 |
[M⊙] | [M⊙] | [M⊙] | [d] | [1011 cm] | [M⊙] | [km s-1] | |||
|
|||||||||
ms_20a | 0.70 | 2.00 | 0.74 | 0.98 | 3.72 | 3.06 | 0.181 | 51.01 | disk instability |
ms_20b | 0.90 | 2.00 | 1.17 | 0.46 | 2.40 | 2.75 | 0.105 | 58.78 | disk instability |
ms_22a | 0.80 | 2.20 | 1.21 | 0.29 | 1.77 | 2.72 | 0.173 | 105.29 | weak H-shell flash |
ms_20c | 0.80 | 2.00 | 1.22 | 0.56 | 2.74 | 2.71 | 0.171 | 64.32 | weak H-shell flash |
ms_24a | 0.90 | 2.40 | 1.40 | 0.33 | 1.95 | 2.63 | 0.172 | 94.95 | stable H burning |
ms_20d | 1.00 | 2.00 | 1.40 | 0.57 | 2.83 | 2.63 | 0.113 | 53.32 | weak H-shell flash |
ms_23a | 0.90 | 2.30 | 1.50 | 0.35 | 2.08 | 2.59 | 0.162 | 85.66 | stable H burning |
ms_24b | 1.00 | 2.40 | 1.88 | 0.37 | 2.25 | 2.46 | 0.116 | 66.91 | stable H burning |
ms_28a | 1.10 | 2.80 | 2.00 | 0.33 | 2.11 | 2.43 | 0.159 | 84.50 | optically thick wind |
ms_30a | 1.20 | 3.00 | 2.45 | 0.44 | 2.64 | 2.33 | 0.141 | 65.34 | optically thick wind |
Notes. Mwd and Mc,i are the initial masses of WD and its companion at the beginning of mass transfer, respectively. Mc,f, Pf, af and R2 denote the final mass of companion star, the orbital period, the binary separation and the radius of secondary at the moment of supernova explosion, respectively. Mstripped and vkick are the stripped mass and the kick velocity caused by supernova impact.
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