Enhancing the rate of tidal disruptions of stars by a self-gravitating disc around a massive central black hole

0385878 - ASÚ 2014 FR eng C - Konferenční příspěvek (zahraniční konf.)
Karas, Vladimír - Šubr, L.
Enhancing the rate of tidal disruptions of stars by a self-gravitating disc around a massive central black hole.
Tidal Disruption Events and AGN Outbursts. Les Ulis: EDP Sciences, 2012 - (Saxton, R.), 01003/1-01003/4. EPJ Web of Conferences, 39. ISSN 2100-014X.
[Tidal Disruption Events and AGN Outbursts. Madrid (ES), 25.6.2012-27.6.2012]
Institucionální podpora: RVO:67985815
Klíčová slova: black holes * accretion disks
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

We further study the idea that a self-gravitating accretion disc around a supermassive black hole can increase the rate of gradual orbital decay of stellar trajectories (and hence tidal disruption events) by setting some stars on eccentric trajectories. Cooperation between the gravitational field of the disc and the dissipative environment can provide a mechanism explaining the origin of stars that become bound tightly to the central black hole.
Trvalý link: http://hdl.handle.net/11104/0215961