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• W174417561 abstract "We consider the fate of a dense cluster of compact stars — neutron stars or stellar-mass black holes — embedded in the nucleus of an active galaxy. The combined effects of two-body dynamical relaxation (the “gravothermal catastrophe”) and star-star collisions and coalescence can drive such a cluster to a relativistic state in a Hubble time. When the core becomes sufficiently relativistic, the cluster inevitably undergoes catastrophic gravitational collapse to a supermassive black hole. This process leads naturally to the birth of supermassive black holes of the “right size” to explain quasars and AGNs: 106 ≲ M/M⊙ ≲ 109." @default.
• W174417561 created "2016-06-24" @default.
• W174417561 creator A5034590981 @default.
• W174417561 date "1986-01-01" @default.
• W174417561 modified "2023-09-27" @default.
• W174417561 title "The Birth of AGNs and Quasars via the Collapse of Dense Star Clusters to Supermassive Black Holes" @default.
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• W174417561 doi "https://doi.org/10.1007/978-94-009-4562-3_9" @default.
• W174417561 hasPublicationYear "1986" @default.
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