Neutron Star观测综述——基于X射线天文台观测
天体物理学
2007-05-23 v1
摘要
我们对X射线天文台对中子星的观测进行简要综述，重点关注中子星所在的超新星遗迹。早期的X射线天文台结果清晰地表明，角分辨率的重要性在于分离中子星辐射与周围星云之间的辐射。
引用
@article{arxiv.astro-ph/0209017,
title = {Chandra Observations of Neutron Stars -- An Overview},
author = {M. C. Weisskopf},
journal= {arXiv preprint arXiv:astro-ph/0209017},
year = {2007}
}
备注
6 pages, 11 figures. To appear in the Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef, eds W. Becker, H. Lesch & J. Truemper. Proceedings are available as MPE-Report 278