毫秒级河外射电暴作为磁星耀发
高能天体物理现象
2013-07-19 v1
摘要
Thornton 等人（2013）发现的毫秒级河外射电暴群体的性质，与我们在 Lorimer 等人（2007）首次观测到河外毫秒射电暴后提出的假设高度吻合，即此类事件与磁星超耀发（hyperflares）有关。我们还指出，Rubio-Herrera 等人（2013）发现的来自 M31 的部分多重毫秒射电暴也可能与较弱的磁星耀发有关。
引用
@article{arxiv.1307.4924,
title = {Millisecond extragalactic radio bursts as magnetar flares},
author = {S. B. Popov and K. A. Postnov},
journal= {arXiv preprint arXiv:1307.4924},
year = {2013}
}
备注
4 pages, no figures; This note is based on the Comment published on-line in the Science magazine. The note is submitted only to the arXiv, and should be cited by its arXiv identifier