新型星族合成模型：密近双白矮星星族的初步结果
太阳与恒星天体物理
2015-03-17 v2
摘要
本文介绍了用于模拟单星和双星演化的软件包 SeBa 的更新，其中实现了新的恒星演化轨迹。SeBa 被应用于研究密近双白矮星星族以及可能导致 Ia 型超新星的双白矮星并合的延迟时间分布。
引用
@article{arxiv.1101.2787,
title = {New population synthesis model: Preliminary results for close double white dwarf populations},
author = {Silvia Toonen and Gijs Nelemans and Simon Portegies Zwart},
journal= {arXiv preprint arXiv:1101.2787},
year = {2015}
}
备注
4 pages, 4 figures, appeared in proceedings for "The 17th European White Dwarf Workshop", shorter version appeared in proceedings for "Binary Star Evolution: Mass Loss, Accretion and Mergers"