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类星体的多样性通过增积和方向统一

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
概括

爱丁顿比,黑洞积累的度量,驱动类星体属性被称为 Eigenvector 1. 类星体的多样性是由埃丁顿比率和观测方向解释的,揭示了一个盘状的气体几何.

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