The core-degenerate scenario for the progenitors of type Ia supernovae
Bo Wang, Weihong Zhou, Zhaoyu Zuo, Yinbi Li, Xia Luo, Jujia Zhang,, Dongdong Liu, Chengyuan Wu

TL;DR
This study investigates the core-degenerate scenario for type Ia supernovae progenitors using binary population synthesis, finding it can account for a subset of observed SNe Ia with specific delay times and metallicity dependence.
Contribution
It provides a detailed analysis of the core-degenerate scenario's viability, including birthrates, delay times, and metallicity effects, which were previously uncertain.
Findings
SN Ia delay times range from 90 Myr to 2.5 Gyr.
Galactic birthrates from this scenario are up to 20% of total SNe Ia.
SNe Ia with circumstellar material constitute 0.7-10% of total SNe Ia.
Abstract
The origin of the progenitors of type Ia supernovae (SNe Ia) is still uncertain. The core-degenerate (CD) scenario has been proposed as an alternative way for the production of SNe Ia. In this scenario, SNe Ia are formed at the final stage of common-envelope evolution from a merger of a carbon-oxygen white dwarf (CO WD) with the CO core of an asymptotic giant branch companion. However, the birthrates of SNe Ia from this scenario are still not well determined. In this work, we performed a detailed investigation on the CD scenario based on a binary population synthesis approach. The SN Ia delay times from this scenario are basically in the range of 90Myr-2500Myr, mainly contributing to the observed SNe Ia with short and intermediate delay times although this scenario can also produce some old SNe Ia. Meanwhile, our work indicates that the Galactic birthrates of SNe Ia from this scenario…
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