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Updated: Feb 22, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
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巨大なブラックホールの近隣環境は 放射性フィードバックによって形作られています

Claudio Ricci1,2,3, Benny Trakhtenbrot4, Michael J Koss4,5

  • 1Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile.

Nature
|September 30, 2017
PubMed
まとめ

超大質量ブラックホールの 放射性フィードバックは 遮蔽ガスと塵を制御します このフィードバックは,質量正常化増量率によって駆動され,ブラックホールのパーセック内の環核物質をクリアします.

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