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Updated: Feb 19, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
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恒星質量ブラックホールの蓄積からの硬いX線で見られる反響の遅延

Bei You1, Wei Yu2,3, Adam Ingram4

  • 1Department of Astronomy, School of Physics and Technology, Wuhan University, Wuhan, China. youbei@whu.edu.cn.

Nature communications
|February 17, 2026
PubMed
まとめ

科学者は,恒星質量ブラックホールX線バイナリでコンプトン・ハンプ・レバーバーを検知し,X線レバーバーと,活発な銀河核とX線バイナリで至る所に存在する蓄積過程を確認した.

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