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Wandering Supermassive Black Holes in Milky-Way-mass Halos

Abstract : We present a self-consistent prediction from a large-scale cosmological simulation for the population of “wandering” supermassive black holes (SMBHs) of mass greater than 106 M on long-lived, kpc-scale orbits within Milky Way (MW)-mass galaxies. We extract a sample of MW-mass halos from the ROMULUS25 cosmological simulation, which is uniquely able to capture the orbital evolution of SMBHs during and following galaxy mergers. We predict that such halos, regardless of recent merger history or morphology, host an average of 5.1 ± 3.3 SMBHs, including their central black hole, within 10 kpc from the galactic center and an average of 12.2 ± 8.4 SMBHs total within their virial radius, not counting those in satellite halos. Wandering SMBHs exist within their host galaxies for several Gyr, often accreted by their host halo in the early Universe. We find, with >4σ significance, that wandering SMBHs are preferentially found outside of galactic disks.
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Contributor : Nathalie POTHIER Connect in order to contact the contributor
Submitted on : Monday, August 8, 2022 - 3:38:10 PM
Last modification on : Tuesday, August 9, 2022 - 3:45:02 AM

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Michael Tremmel, Fabio Governato, Marta Volonteri, Andrew Pontzen, Thomas R. Quinn. Wandering Supermassive Black Holes in Milky-Way-mass Halos. The Astrophysical Journal Letters, 2018, 857, ⟨10.3847/2041-8213/aabc0a⟩. ⟨insu-03747705⟩



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