Results 1 to 10 of about 5,978,686 (296)

Fast-moving stars around an intermediate-mass black hole in ω Centauri. [PDF]

open access: yesNature
Black holes have been found over a wide range of masses, from stellar remnants with masses of 5-150 solar masses (Msun), to those found at the centers of galaxies with $M>10^5$ Msun. However, only a few debated candidate black holes exist between 150 and
Häberle M   +17 more
europepmc   +6 more sources

Intermediate-mass black hole binary evolution in nuclear star clusters: The effect of the stellar-mass black hole population

open access: yesAstronomy & Astrophysics
Aims. In this study, we investigate the dynamics of intermediate-mass black hole (IMBH) binaries within nuclear star clusters (NSCs) that contain a population of stellar-mass black holes (BHs).
Khan Fazeel Mahmood   +6 more
doaj   +3 more sources

An Intermediate-mass Black Hole Hidden behind Thick Obscuration

open access: yesThe Astrophysical Journal
Recent models suggest approximately half of all accreting supermassive black holes (SMBHs; M _BH ≳ 10 ^5 M _⊙ ) are expected to undergo intense growth phases behind Compton-thick ( N _H > 1.5 × 10 ^24 cm ^−2 ) veils of obscuring gas.
Peter G. Boorman   +14 more
doaj   +5 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

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.
Greene, Jenny E.   +2 more
openaire   +2 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.
Kayhan Gültekin   +9 more
openaire   +2 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 ...
Miller, M. Coleman, Colbert, E. J. M.
openaire   +2 more sources

Partial Tidal Disruptions of Main-sequence Stars by Intermediate-mass Black Holes

open access: yesThe Astrophysical Journal, 2023
We study close encounters of a 1 M _⊙ middle-age main-sequence star (modeled using MESA) with massive black holes through hydrodynamic simulations, and explore in particular the dependence of the outcomes on the black hole mass.
Fulya Kıroğlu   +5 more
doaj   +1 more source

Constraints on Galactic intermediate mass black holes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
Intermediate Mass Black Holes (IMBHs; 10^1.3-5 M_sun) are thought to form as relics of Population III stars or from the runaway collapse of stars in young clusters; their number and very existence are uncertain. We ran N-body simulations of Galactic IMBHs, modelling them as a halo population distributed according to a Navarro, Frenk & White (NFW ...
Mapelli, M., FERRARA, ANDREA, Rea, N.
openaire   +2 more sources

Constraining a Companion of the Galactic Center Black Hole Sgr A*

open access: yesThe Astrophysical Journal, 2023
We use 23 yr of astrometric and radial velocity data on the orbit of the star S0-2 to constrain a hypothetical intermediate-mass black hole orbiting the massive black hole Sgr A* at the Galactic center.
Clifford M. Will   +6 more
doaj   +1 more source

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