Is SN 2006X from a WD + MS system with optically thick wind?
Solar and Stellar Astrophysics
2014-11-20 v1
Abstract
The single-degenerate channel is widely accepted as the progenitors of type Ia supernovae (SNe Ia). Following the work of Meng, Chen and Han (2009), we reproduced the birth rate and age of supernovae like SN 2006X by the single-degenerate model (WD + MS) with an optically thick wind, which may imply that the progenitor of SN 2006X is a WD + MS system.
Cite
@article{arxiv.0910.1915,
title = {Is SN 2006X from a WD + MS system with optically thick wind?},
author = {Xiangcun Meng and Wuming Yang and Xuemin Geng},
journal= {arXiv preprint arXiv:0910.1915},
year = {2014}
}
Comments
10 pages, 2 figures, accepted for publication in NewA