2021
DOI: 10.48550/arxiv.2108.07439
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Hot subdwarfs from the surviving companions of the white dwarf + main-sequence channel of Type Ia supernovae

Xiangcun Meng,
Yangpin Luo

Abstract: Some surviving companions of type Ia supernovae (SNe Ia) from the white-dwarf + main-sequence (WD + MS) channel may evolve to hot subdwarfs. In this paper, we preformed stellar evolution calculations for surviving companions of close WD + MS systems in the spin-up/spin-down model and the canonical non-rotating model to map out the initial parameter spaces in the orbital period -secondary mass plane in which the surviving companions can evolve to hot subdwarfs. Based on these results, we carried out a series of… Show more

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