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Updated: Nov 21, 2025

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
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一个明亮的γ射线耀斑被解释为NGC 253中的巨型磁星耀斑

D Svinkin1, D Frederiks2, K Hurley3

  • 1Ioffe Institute, St Petersburg, Russia. svinkin@mail.ioffe.ru.

Nature
|January 14, 2021
PubMed
概括

从磁星,高度磁化的中子星, 产生强大的X射线和马射线的爆发. 研究人员观察到GRB 200415A,确定它是NGC 253星系中的磁星.

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