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Growth of Super-Massive Black Holes in Galaxy Nuclei
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Françoise Combes
(
- Paris Observatory
Abstract
Black holes and galaxies appear to grow in symbiosis. Non-axisymmetric features like bars, and even several embedded density waves in galaxies are necessary to exchange angular momentum and drive the gas to feed the nucleus, Feedback regulates star formation, and can be of radiative or kinetic modes in origin. Gas outflows are energy-driven at the beginning and may become momentum driven, with lower efficiency. If the regulation appears to work quite well in galaxy clusters to regulate cooling flows, it is still debated in individual galaxies.
Related research groups
Growth of Super-Massive Black Holes in Galaxy Nuclei
Venue
Higgs Centre Seminar Room, JCMB
(Find us on campus maps)
The Higgs Centre for Theoretical Physics
School of Physics and Astronomy
James Clerk Maxwell Building, 4305
Peter Guthrie Tait Road
Edinburgh
EH9 3FD
UK
School of Physics and Astronomy
James Clerk Maxwell Building, 4305
Peter Guthrie Tait Road
Edinburgh
EH9 3FD
UK
Online
Zoom
The speaker of the colloquium will join remotely.
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