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SSS17aが二重中性子星の合併の結果であることを示す電磁的証拠

C D Kilpatrick1, R J Foley2, D Kasen3,4

  • 1Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA. cdkilpat@ucsc.edu.

Science (New York, N.Y.)
|October 18, 2017
PubMed
まとめ

引力波 (GW170817) で検出された2つの中性子星の融合により,光学的トランジエンント (SSS17a) が生成された. このキロノヴァの発生は 急速な中性子捕獲によって加速され 二重中性子星の 融合の起源が確認されました

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