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Updated: Apr 24, 2026

Methods for Measuring the Orientation and Rotation Rate of 3D-printed Particles in Turbulence
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集積と方向によって統一されたクエサールの多様性

Yue Shen1, Luis C Ho2

  • 11] Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California 91101, USA [2] Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China.

Nature
|September 12, 2014
PubMed
まとめ

ブラックホールの増殖を測るエディントン比は,イゲインベクター1として知られるクワザーの性質を駆動する. クワザーの多様性は,エディントン比率と観測方向によって説明され,円盤のようなガスの幾何学を明らかにします.

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