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Updated: May 27, 2026

Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
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Published on: July 2, 2012

異例のG-ray burst GRB 101225Aは,ヘリウム星/中性子星が赤道偏移0.33で合体したことから発生した

C C Thöne1, A de Ugarte Postigo, C L Fryer

  • 1IAA - CSIC, Glorieta de la Astronomía s/n, 18008 Granada, Spain. cthoene@iaa.es

Nature
|December 2, 2011
PubMed
まとめ

異常な長いガンマ線爆発 (GRB) 101225Aは,熱X線トランジタと光学超新星に続く長寿の放射を示した. ヘリウム星と中性子星の融合が原始イベントとして提案されている.

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