Number of the records: 1  

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

  1. 1.
    0385878 - ASÚ 2014 FR eng C - Conference Paper (international conference)
    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]
    Institutional support: RVO:67985815
    Keywords : black holes * accretion disks
    Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

    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.
    Permanent Link: http://hdl.handle.net/11104/0215961

     
     
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.