论文标题
单个二进制可以托管复发的热核超新星
A Single Binary May Host Recurrent Thermonuclear Supernovae
论文作者
论文摘要
IAX型超新星（SNE IAX）最常见的祖细胞系统是从非分级氦供体星中积聚的近chandrasekhar-Mass White Dwarf（WD）的部分偏移，在爆炸后留下了边界的造物。在本文中，我们研究了WD Remant在系统一生中是否可以经历多个SNE。我们使用用于天体物理学（MESA）实验的模块来进化各种单对二元二进制文件，以确定由于多个氦积聚阶段，哪些可能会发生多个SNE IAX。我们还研究了双WD系统形成后随后的IA SN类型SN的可能性。我们的工作得出的结论是，用相对较高的质量供体关闭二进制文件，对于几种热核SNE产生的可能性最高。
The most commonly accepted progenitor system for Type Iax supernovae (SNe Iax) is the partial deflagration of a near-Chandrasekhar-mass white dwarf (WD) accreting from a non-degenerate helium donor star, leaving a bound remnant following the explosion. In this paper, we investigate whether the WD remant can undergo multiple SNe during the system's lifetime. We use Modules for Experiments in Astrophysics (MESA) to evolve various single-degenerate binaries to determine which could plausibly undergo multiple SNe Iax due to multiple helium accretion phases. We also investigate the possibility for a subsequent Type Ia SN after the formation of a double WD system. Our work concludes that close binaries with relatively high-mass donors produce the highest probability for several thermonuclear SNe.
