Cold, clumpy accretion onto an active supermassive black hole

Cold, clumpy accretion onto an active supermassive black hole

Supermassive black holes in galaxy centres can grow by the accretion of gas, liberating energy that might regulate star formation on galaxy-wide scales. The nature of the gaseous fuel reservoirs that power black hole growth is nevertheless largely unconstrained by observations, and is instead routin...

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Bibliographic Details
Main Authors: Tremblay, Grant R., Oonk, J. B. Raymond, Combes, Françoise, Salomé, Philippe, Christopher, Philippe, O’Dea, P., Baum, Stefi A., Voit, G. Mark, Donahue, Megan, McNamara, Brian R., Davis, Timothy A., McDonald, Michael A., Edge, Alastair C., Clarke, Tracy E., Galván-Madrid, Roberto, Bremer, Malcolm N., Edwards, Louise O. V., Fabian, Andrew C., Hamer, Stephen, Li, Yuan, Maury, Anaëlle, Russell, Helen R., Quillen, Alice C., Urry, C. Megan, Sanders, Jeremy S., Wise, Michael W.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: Nature Publishing Group 2017
Online Access:http://hdl.handle.net/1721.1/108337
https://orcid.org/0000-0001-5226-8349

Internet

http://hdl.handle.net/1721.1/108337
https://orcid.org/0000-0001-5226-8349

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