Tidal Disruption of a Main Sequence Star by a Super-massive Black Hole Binary

Details Tidal Disruption of a Main Sequence Star by a Super-massive Black Hole Binary Tidal Disruption of a Main Sequence Star by a Super-massive Black Hole Binary

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.j8003a&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #J8.003

Physics

Scientific paper

We present results from a numerical relativity study of the tidal disruption of a main sequence star by a super-massive black hole binary during coalescence. We compare the disruption process with the traditional case of a single massive black hole. In particular, we focus on the geometry of the ejecta and the fall back rate of the debris. We also elaborate on the observational signatures and the possibility of detecting the tidal flares from these disruptive encounters.

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