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- W3100911930 abstract "We compute rates of tidal disruption of stars by supermassive black holes in galactic nuclei, using downwardly revised black hole masses from the MBH-σ relation. In galaxies with steep nuclear density profiles, which dominate the overall event rate, the disruption frequency varies inversely with assumed black hole mass. We compute a total rate for nondwarf galaxies of ~10-5 yr-1 Mpc-3, about a factor of 10 higher than in earlier studies. Disruption rates are predicted to be highest in nucleated dwarf galaxies, assuming that such galaxies contain black holes. Monitoring of a rich galaxy cluster for a few years could rule out the existence of intermediate-mass black holes in dwarf galaxies." @default.
- W3100911930 created "2020-11-23" @default.
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- W3100911930 date "2004-01-01" @default.
- W3100911930 modified "2023-10-13" @default.
- W3100911930 title "Revised Rates of Stellar Disruption in Galactic Nuclei" @default.
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- W3100911930 doi "https://doi.org/10.1086/379767" @default.
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