Supernova Ia Remnants with M-dwarf Surviving Companions
We study the possibility that Type Ia supernovae might be produced by binary systems where the companion of the exploding white dwarf is an M-dwarf star. Such a companion would appear as a runaway star, retaining its pre-explosion orbital velocity along with a kick imparted by the supernova ejecta. It might be rapidly rotating, from being tidally
Pan, Kuo-Chuan et al.
Fecha de publicación:
1
2026