中子星的磁场
高能天体物理现象
2017-09-27 v1
摘要
本文简要回顾了我们对中子星磁场演化的现有理解，这基本上决定了不同观测类别中子星之间的演化路径。本文重点在于双星系统中的演化以及新出现的毫秒脉冲星类别。
引用
@article{arxiv.1709.07106,
title = {Magnetic Fields of Neutron Stars},
author = {Sushan Konar},
journal= {arXiv preprint arXiv:1709.07106},
year = {2017}
}
备注
Has appeared in Journal of Astrophysics and Astronomy special issue on 'Physics of Neutron Stars and Related Objects', celebrating the 75th birth-year of G. Srinivasan