This video describes a fundamental element in our understanding of the evolution of active galaxies with powerful jets. Originally counter-rotating black holes experience an absence of the Bardeen-Petterson effect at zero black hole spin. A new plane of accretion is then formed which is tilted with respect to the previous phase and this has implications for feedback on star formation and stellar velocity dispersion in the bulge. Video courtesy of Kennesaw State University physics major Michael Williams.
Негізгі бет Counter-rotating black holes and a tilted accretion disk at zero spin
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