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Black hole demographics from the M bullet - relation

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Merritt, D., Ferrarese, L.·2001·Monthly Notices of the Royal Astronomical Society

Abstract

We analyse a sample of 32 galaxies for which a dynamical estimate of the mass of the hot stellar component, Mbulge, is available. For each of these galaxies, we calculate the mass of the central black hole, M●, using the tight empirical correlation between M● and bulge stellar velocity dispersion. The frequency function N[log(M● / Mbulge)] is reasonably well described as a Gaussian with 〈log(M● / Mbulge)〉 ≈ − 2.90 and standard deviation ∼0.45; the implied mean ratio of black hole mass to bulge mass is a factor of ∼5 smaller than generally quoted in the literature. We present marginal evidence for a lower, average black hole mass fraction in more massive galaxies. The total mass density in black holes in the local Universe is estimated to be ∼5 × 105 M⊙ Mpc −3, consistent with that inferred from high-redshift (z ∼ 2) active galactic nuclei.

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Metadata

Authors
Merritt, D., & Ferrarese, L.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2001-01-21
Volume
320
Issue
3
Pages
L30-L34
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W1673152325
Cited by
329
References
0
FWCI
26.47
Type
journal article
Language
en
Open access
green

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Merritt, D., & Ferrarese, L. (2001). Black hole demographics from the M bullet - relation. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2001.04165.x

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