吸积单星中子星的空间分布
天体物理学
2016-02-10 v1
摘要
我们在此报告了由旧单星中子星（OINSS）从星际介质（ISM）吸积产生的亮度分布的计算机模型。我们显示，对于不同平均速度的OINSS，亮度分布呈环形结构，最大值约为5 kpc。
引用
@article{arxiv.astro-ph/9609126,
title = {Spatial distribution of accreting isolated neutron stars},
author = {S. B. Popov and M. E. Prokhorov},
journal= {arXiv preprint arXiv:astro-ph/9609126},
year = {2016}
}
备注
8 pages, 9 PostScript figures, to be presented as a poster at the conference "Current problems in astrophysics", Moscow, September 23-28, 1996. Short version will be published in Astronomical and Astrophysical Transactions