Tidal disruption of white dwarfs by intermediate mass black holes
Modeling ultra-close encounters between a white dwarf and a spinning, intermediate mass black hole requires a full general relativistic treatment of gravity. This paper summarizes results from such a study. Our results show that the disruption process and prompt accretion of the debris strongly depe...
Main Authors: | Bode T., Shcherbakov R.V., Haas R., Laguna P. |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2012-12-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20123907002 |
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