软伽马射线重复暴与反常X射线脉冲星作为高度磁化白矮星
太阳与恒星天体物理
2016-03-02 v1 高能天体物理现象
摘要
我们表明，软伽马射线重复暴（SGRs）与反常X射线脉冲星（AXPs）可被解释为近期提出的高度磁化白矮星（B-WDs）。B-WDs的半径与磁场完全足以将SGRs/AXPs中的能量解释为自转供能。而高度磁化中子星需要额外的、观测上尚未充分确立的能源；磁化白矮星则遵循钱德拉塞卡理论（C-WDs），表现出大的紫外光度，而观测通过严格的上限对其进行了约束。
引用
@article{arxiv.1603.00141,
title = {Soft gamma-ray repeaters and anomalous X-ray pulsars as highly magnetized white dwarfs},
author = {Banibrata Mukhopadhyay and A. R. Rao},
journal= {arXiv preprint arXiv:1603.00141},
year = {2016}
}
备注
6 pages including 1 figure; to appear in the Proceedings of 14th Marcel Grossman Meeting (MG14), Rome, Italy, 12-18 July 2015; based on the talk given in the meeting in the session WD2