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Intermediate-Mass Black Holes: The Essential Population to Explore the Unified Model for Accretion and Ejection Processes

open access: yesGalaxies, 2023
We study radio and X-ray emissions from intermediate-mass black holes (IMBHs) and explore the unified model for accretion and ejection processes. The radio band survey of IMBH (candidate) hosted galaxies indicates that only a small fraction (∼0.6%) of ...
Xiaolong Yang, Jun Yang
doaj   +3 more sources

Intermediate-Mass Black Holes [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2020
We describe ongoing searches for intermediate-mass black holes with M BH ≈ 10–10 5 M ⊙ . We review a range of search mechanisms, both dynamical and those that rely on accretion signatures.
Luis Ho, Jay Strader, Jenny Greene
exaly   +3 more sources

Intermediate-mass black holes and the Fundamental Plane of black hole accretion

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT We present new 5 GHz Very Large Array observations of a sample of eight active intermediate-mass black holes with masses 104.9 M⊙ < M < 106.1 M⊙ found in galaxies with stellar masses M* < 3 × 109 M⊙. We detected five of the eight sources at high significance.
Amy Reines   +2 more
exaly   +3 more sources

Mass Measurements of Stellar and Intermediate-Mass Black Holes [PDF]

open access: yesSpace Science Reviews, 2013
28 pages, 12 figures. Accepted for publication in Space Science Reviews (DOI 10.1007/s11214-013-0030-6). Also to appear in hard cover in the Space Sciences Series of ISSI "The Physics of Accretion onto Black Holes" (Springer Publisher).
Jorge Casares   +2 more
exaly   +7 more sources

INTERMEDIATE-MASS BLACK HOLES [PDF]

open access: yesInternational Journal of Modern Physics D, 2004
The mathematical simplicity of black holes, combined with their links to some of the most energetic events in the universe, means that black holes are key objects for fundamental physics and astrophysics. Until recently, it was generally believed that black holes in nature appear in two broad mass ranges: stellar-mass (M~3–20 M⊙), which are produced ...
Cole Miller
exaly   +3 more sources

Mechanism for the suppression of intermediate-mass black holes [PDF]

open access: yesAstronomy Letters, 2010
A model for the formation of supermassive primordial black holes in galactic nuclei with the simultaneous suppression of the formation of intermediate-mass black holes is presented. A bimodal mass function for black holes formed through phase transitions in a model with a "Mexican hat" potential has been found.
Yury Eroshenko   +2 more
exaly   +3 more sources

On the dynamic formation of accreting intermediate-mass black holes [PDF]

open access: yesAstronomical and Astrophysical Transactions, 2007
We compute the probability that intermediate mass black holes (IMBHs) capture companions due to dynamical interactions and become accreting sources, and explore the possibility that the accreting IMBHs would appear as ultra-luminous X-ray sources (ULXs). We focus on IMBHs originating from low-metallicity Population III stars.
Konstantin Postnov   +2 more
exaly   +3 more sources

Rapid Intermediate-mass Black Hole Formation via Runaway Mergers of Black Holes

open access: yesThe Astrophysical Journal Letters
Observations indicate that supermassive black holes in high-redshift galaxies formed on timescales far shorter than classical growth models allow. One hypothesis suggests intermediate-mass black hole (IMBH) seeds as an efficient growth channel.
Yining Sun, Long Wang
doaj   +3 more sources

Simulating the growth of intermediate-mass black holes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Accepted for publication in ...
Pacucci, Fabio, Ferrara, Andrea
openaire   +2 more sources

Intermediate-mass black holes in globular clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2012
Abstract There have been reports of possible detections of intermediate-mass black holes (IMBHs) in globular clusters (GCs). Empirically, there exists a tight correlation between the central supermassive black hole (SMBH) mass and the mean velocity dispersion of elliptical galaxies, ‘pseudo-bulges’ and classical bulges of spiral galaxies.
Lou, Yu-Qing, Wu, Yi-Hong
openaire   +2 more sources

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