The Impact of Bound Stellar Orbits and General Relativity on the Temporal Behavior of Tidal Disruption Flares
We have carried out general relativistic particle simulations of stars tidally disrupted by massive black holes. When a star is disrupted in a bound orbit with moderate eccentricity instead of a parabolic orbit, the temporal behavior of the resulting stellar debris changes qualitatively. The debris...
Saved in:
Published in | arXiv.org |
---|---|
Main Authors | , , |
Format | Paper Journal Article |
Language | English |
Published |
Ithaca
Cornell University Library, arXiv.org
18.09.2013
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Be the first to leave a comment!