中子星非理想强磁性等离子体及其电磁辐射
天体物理学
2008-11-26 v3
摘要
我们研究了构成磁性中子星外层包层的非理想、强磁性等离子体的状态方程、极化和辐射特性。针对部分电离的氢大气以及氢或铁凝聚表面，进行了详细计算。这篇论文是astro-ph/0511803的配套论文。
引用
@article{arxiv.astro-ph/0512086,
title = {New evidence for strong nonthermal effects in Tycho's supernova remnant},
author = {H. J. Voelk and E. G. Berezhko and L. T. Ksenofontov},
journal= {arXiv preprint arXiv:astro-ph/0512086},
year = {2008}
}
备注
5 pages, 4 figures. Accepted for publication in Astrophysics and Space Science, Proc. of "The Multi-Messenger Approach to High-Energy Gamma-ray Sources (Third Workshop on the Nature of Unidentified High-Energy Sources)", Barcelona, July 4-7, 2006