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Updated: Jun 25, 2025

Magnetically Induced Rotating Rayleigh-Taylor Instability
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超大質量ブラックホールが恒星を破壊した後のレンズ・ティリング前行

Dheeraj R Pasham1, Michal Zajaček2, C J Nixon3

  • 1Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA. drreddy@mit.edu.

Nature
|May 22, 2024
PubMed
まとめ

天文学者は,潮乱 (TDE) による準周期的なX線信号を観測した. これらの信号は,ブラックホールのスピンによる相対的なトルクが,黒穴のダイナミクスの洞察を提供して,蓄積円盤のプレッシャーを引き起こしていることを示唆しています.

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