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Detection of Gravitational Wave Emission by Supermassive Black Hole Binaries Through Tidal Disruption Flares
Galaxy mergers produce supermassive black hole binaries, which emit gravitational waves prior to their coalescence. We perform three-dimensional hydrodynamic simulations to study the tidal disruption of stars by such a binary in the final centuries of its life. We find that the gas stream of the ste...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Nature Publishing Group
2016
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5073286/ https://www.ncbi.nlm.nih.gov/pubmed/27767188 http://dx.doi.org/10.1038/srep35629 |