1 code implementation • 1 Aug 2018 • Grant R. Tremblay, Françoise Combes, J. B. Raymond Oonk, Helen R. Russell, Michael A. McDonald, Massimo Gaspari, Bernd Husemann, Paul E. J. Nulsen, Brian R. McNamara, Stephen L. Hamer, Christopher P. O'Dea, Stefi A. Baum, Timothy A. Davis, Megan Donahue, G. Mark Voit, Alastair C. Edge, Elizabeth L. Blanton, Malcolm N. Bremer, Esra Bulbul, Tracy E. Clarke, Laurence P. David, Louise O. V. Edwards, Dominic A. Eggerman, Andrew C. Fabian, William R. Forman, Christine Jones, Nathaniel Kerman, Ralph P. Kraft, Yuan Li, Meredith C. Powell, Scott W. Randall, Philippe Salomé, Aurora Simionescu, Yuanyuan Su, Ming Sun, C. Megan Urry, Adrian N. Vantyghem, Belinda J. Wilkes, John A. ZuHone
The entire scenario is therefore consistent with a galaxy-spanning "fountain", wherein cold gas clouds drain into the black hole accretion reservoir, powering jets and bubbles that uplift a cooling plume of low-entropy multiphase gas, which may stimulate additional cooling and accretion as part of a self-regulating feedback loop.
Astrophysics of Galaxies
1 code implementation • 7 Jun 2016 • Grant R. Tremblay, J. B. Raymond Oonk, Françoise Combes, Philippe Salomé, Christopher P. O'Dea, Stefi A. Baum, G. Mark Voit, Megan Donahue, Brian R. McNamara, Timothy A. Davis, Michael A. McDonald, Alastair C. Edge, Tracy E. Clarke, Roberto Galván-Madrid, Malcolm N. Bremer, Louise O. V. Edwards, Andrew C. Fabian, Stephen L. Hamer, Yuan Li, Anaëlle Maury, Helen R. Russell, Alice C. Quillen, C. Megan Urry, Jeremy S. Sanders, Michael Wise
Supermassive black holes in galaxy centres can grow by the accretion of gas, liberating energy that might regulate star formation on galaxy-wide scales.
Astrophysics of Galaxies High Energy Astrophysical Phenomena