吸积的孤立致密天体辐射功率分布
天体物理学
2008-02-03 v2
摘要
我们在银河系中R-Z平面上，对旧的孤立中子星和黑洞从星际介质中吸积产生的辐射功率分布进行计算机建模。我们展示，功率分布呈环形结构，最大值为约5-6千帕克。
引用
@article{arxiv.astro-ph/9705236,
title = {Distribution of the luminosity of accreting isolated compact objects},
author = {S. B. Popov and M. E. Prokhorov},
journal= {arXiv preprint arXiv:astro-ph/9705236},
year = {2008}
}
备注
4 pages, 6 PostScript figures. Uses l-aa style. To be presented as a poster at the conference "Neutron stars - 97", St. Petersburg, June 9-11, 1997. In the replaced version fig. 3 and 5 are changed