S型共生双星中高质量转移比的指征
太阳与恒星天体物理
2017-03-20 v1
摘要
通过模拟掩食S型共生星EG And和SY Mus中的H柱密度，我们推导了来自其巨星的星风速度剖面和相应的质量损失率。我们的分析揭示了在轨道平面上星风的强烈增强。
引用
@article{arxiv.1602.01668,
title = {Indication of the High Mass-Transfer Ratio in S-type Symbiotic Binaries},
author = {Natalia Shagatova and Augustin Skopal},
journal= {arXiv preprint arXiv:1602.01668},
year = {2017}
}
备注
proceedings of the conference "The Physics of Evolved Stars: a Conference Dedicated to the Memory of Olivier Chesneau", 2 pages, 2 figures