Chaotic cold accretion on to black holes in rotating atmospheres

The fueling of black holes is one key problem in the evolution of baryons in the universe. Chaotic cold accretion (CCA) profoundly differs from classic accretion models, as Bondi and thin disc theories. Using 3D high-resolution hydrodynamic simulations, we now probe the impact of rotation on the hot...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2015-07, Vol.579, p.A62
Hauptverfasser:	Gaspari, M., Brighenti, F., Temi, P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Accretion disks Atmospheres black hole physics Black holes (astronomy) Chaos theory Cold working Feedback galaxies: ISM hydrodynamics instabilities Three dimensional turbulence
Online-Zugang:	Volltext
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