Results 31 to 40 of about 1,494,639 (351)

Population statistics of intermediate-mass black holes in dwarf galaxies using the newhorizon simulation [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
While it is well established that supermassive black holes (SMBHs) co-evolve with their host galaxy, it is currently less clear how lower-mass black holes, so-called intermediate-mass black holes (IMBHs), evolve within their dwarf galaxy hosts. In this
R. Beckmann   +8 more
semanticscholar   +1 more source

A Sample of Massive Black Holes in Dwarf Galaxies Detected via [Fe x] Coronal Line Emission: Active Galactic Nuclei and/or Tidal Disruption Events [PDF]

open access: yesAstrophysical Journal, 2021
The massive black hole (BH) population in dwarf galaxies (M BH ≲ 105 M ⊙) can provide strong constraints on the origin of BH seeds. However, traditional optical searches for active galactic nuclei (AGNs) only reliably detect high-accretion, relatively ...
M. Molina   +4 more
semanticscholar   +1 more source

Constraints on primordial black holes from observation of stars in dwarf galaxies [PDF]

open access: yes, 2022
We propose a way to constrain the primordial black hole (PBH) abundance in the range of PBH masses $m$ around $10^{20}$g based on their capture by Sun-like stars in dwarf galaxies, with subsequent star destruction.
Nicolas Esser, P. Tinyakov
semanticscholar   +1 more source

Variability-selected Intermediate-mass Black Hole Candidates in Dwarf Galaxies from ZTF and WISE [PDF]

open access: yesAstrophysical Journal, 2021
While it is difficult to observe the first black hole seeds in the early universe, we can study intermediate-mass black holes (IMBHs) in local dwarf galaxies for clues about their origins.
C. Ward   +11 more
semanticscholar   +1 more source

Transients from ONe White Dwarf – Neutron Star/Black Hole Mergers [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2021
We conduct the first 3D hydrodynamic simulations of oxygen-neon white dwarf-neutron star/black hole mergers (ONe WD-NS/BH mergers). Such mergers constitute a significant fraction, and may even dominate, the inspiral rates of all WD-NS binaries. We post-
A. Bobrick   +4 more
semanticscholar   +1 more source

Modelling quantum aspects of disruption of a white dwarf star by a black hole

open access: yesScientific Reports, 2021
We study the final stages of the evolution of a binary system consisted of a black hole and a white dwarf star. We implement the quantum hydrodynamic equations and carry out numerical simulations.
Tomasz Karpiuk   +3 more
doaj   +1 more source

Relics of Supermassive Black Hole Seeds: The Discovery of an Accreting Black Hole in an Optically Normal, Low Metallicity Dwarf Galaxy [PDF]

open access: yesAstrophysical Journal Letters, 2021
The detection and characterization of supermassive black holes (SMBHs) in local low mass galaxies is crucial to our understanding of the origins of SMBHs.
J. Cann   +13 more
semanticscholar   +1 more source

Two Candidates for Dual AGN in Dwarf-dwarf Galaxy Mergers

open access: yesThe Astrophysical Journal, 2023
Dual active galactic nuclei (DAGN) are important for understanding galaxy-merger-triggered fueling of black holes and the hierarchical growth of structures.
Marko Mićić   +3 more
doaj   +1 more source

A Comparison between the Morphologies and Structures of Dwarf Galaxies with and without Active Massive Black Holes

open access: yesThe Astrophysical Journal, 2023
We study the morphologies and structures of 57 dwarf galaxies that are representative of the general population of dwarf galaxies and compare their demographics to a sample of dwarf galaxies hosting optically selected active galactic nuclei (AGNs).
Seth J. Kimbrell   +3 more
doaj   +1 more source

Dynamical Analysis of the Dark Matter and Central Black Hole Mass in the Dwarf Spheroidal Leo I [PDF]

open access: yesAstrophysical Journal, 2021
We measure the central kinematics for the dwarf spheroidal galaxy Leo I using integrated-light measurements and previously published data. We find a steady rise in the velocity dispersion from 300″ into the center. The integrated-light kinematics provide
Maria Jose Bustamante-Rosell   +6 more
semanticscholar   +1 more source

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