Tidal disruption rate of stars by supermassive black holes obtained by direct N-body simulations

Monthly Notices of the Royal Astronomical Society

Volumn 418, Issue 2, 2011, Pages 1308-1324

  Brockamp, M ^a   Baumgardt, H ^b   Kroupa, P ^a  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF QUEENSLAND   (Australia)

Author keywords

Black hole physics; Gravitational dynamics; Methods: N body simulations; S rsic profiles; Spherical galaxies

Indexed keywords

EID: 81355160485     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19580.x     Document Type: Article

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