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Supermassive Black Hole Spin and Reverberation

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arxiv 1903.05469 v1 pith:OQQX65A6 submitted 2019-03-13 astro-ph.HE

A. Zoghbi , D. R. Wilkins , L. Brenneman , G. Miniutti , G. Matt , J. Garcia , E. Kara , E. Cackett
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B. De Marco M. Dovciak
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classification astro-ph.HE
keywords blackholereverberationarounddetectorsdisk-coronaecho-mappingemerged
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X-ray reverberation mapping has emerged as a powerful probe of microparsec scales around AGN, and with high sensitivity detectors, its full potential in echo-mapping the otherwise inaccessible disk-corona at the black hole horizon scale will be revealed.

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Cited by 1 Pith paper

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  1. Slow and fat: low-spin SMBHs are more massive

    astro-ph.GA 2019-08 conditional novelty 5.0 of 10

    Low-spin supermassive black holes keep growing during the gas-clearing phase because their low radiative efficiency makes feedback less effective, so they end up more massive than high-spin ones at fixed galaxy veloci...

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