脉冲星磁极体内的物理过程及非热高频辐射
天体物理学
2007-05-23 v1
摘要
脉冲星非热辐射的能源为中子星的旋转能量损失。中子星的旋转能量通过一系列长期过程转化为脉冲星辐射。本文讨论了这些过程。
引用
@article{arxiv.astro-ph/9612078,
title = {Physical processes in pulsar magnetospheres and non-thermal high-frequency emission},
author = {Vladimir V. Usov},
journal= {arXiv preprint arXiv:astro-ph/9612078},
year = {2007}
}
备注
8 pages, latex, no figures. To be published in the Proceedings of the IAU Colloquium No 160, Pulsars: Problems and Progress, Sydney, 8-12 January 1996 (invited paper)