X线耀.

Z G Dai1, X Y Wang, X F Wu

  • 1Department of Astronomy, Nanjing University, Nanjing 210093, China. dzg@nju.edu.cn

Science (New York, N.Y.)
|February 25, 2006
PubMed
概括

短时间的马射线爆发可能来自于合并的中子星. 新形成的脉冲星可以在合并事件后通过磁场相互作用产生持久的X射线耀斑.

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