SIMBAD references

2013ApJ...778L..35M - Astrophys. J., 778, L35 (2013/December-1)

Constraining the spin-down timescale of the white dwarf progenitors of type Ia supernovae.

MENG X. and PODSIADLOWSKI P.

Abstract (from CDS):

Justham and Di Stefano et al. proposed that the white dwarf progenitor of a Type Ia supernova (SN Ia) may have to spin down before it can explode. As the white dwarf spin-down timescale is not well known theoretically, here we try to constrain it empirically (within the framework of this spin-down model) for progenitor systems that contain a giant donor and for which circumbinary material has been detected after the explosion: we obtain an upper limit of a few 107yr. Based on the study of Di Stefano & Kilic, this means that it is too early to rule out the existence of a surviving companion in SNR 0509-67.5.

Abstract Copyright:

Journal keyword(s): binaries: symbiotic - stars: evolution - supernovae: general - white dwarfs

Simbad objects: 3

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2021.02.24-22:17:24

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