Results 31 to 40 of about 8,250 (145)

Do Neutron Star Ultraluminous X-Ray Sources Masquerade as Intermediate-mass Black Holes in Radio and X-Ray?

open access: yesThe Astrophysical Journal
Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) intermediate-mass black holes.
Teresa Panurach   +10 more
doaj   +1 more source

Discovery of a Planar Black Hole Mass Scaling Relation for Spiral Galaxies

open access: yesThe Astrophysical Journal Letters, 2023
Supermassive black holes (SMBHs) are tiny in comparison to the galaxies they inhabit, yet they manage to influence and coevolve along with their hosts.
Benjamin L. Davis, Zehao Jin
doaj   +1 more source

The Fate of EMRI-IMRI Pairs in Active Galactic Nucleus Accretion Disks: Hydrodynamical and Three-body Simulations

open access: yesThe Astrophysical Journal
Extreme-mass-ratio inspirals (EMRIs) and intermediate-mass-ratio inspirals (IMRIs) are important gravitational wave (GW) sources for the Laser Interferometer Space Antenna.
Peng Peng   +4 more
doaj   +1 more source

A New Timescale–Mass Scaling for the Optical Variation of Active Galactic Nuclei across the Intermediate-mass to Supermassive Scales

open access: yesThe Astrophysical Journal
The variability of active galactic nuclei (AGNs) has long been servicing as an essential avenue of exploring the accretion physics of a black hole (BH). There are two commonly used methods for analyzing AGN variability.
Zhen-Bo Su   +5 more
doaj   +1 more source

Where are the Intermediate Mass Black Holes? [PDF]

open access: green, 2022
Jillian Bellovary   +9 more
openalex   +1 more source

HOLESOM: Constraining the Properties of Slowly Accreting Massive Black Holes with Self-organizing Maps

open access: yesThe Astrophysical Journal
Accreting massive black holes (MBHs, with M _• > 10 ^3 M _⊙ ) are known for their panchromatic emission, spanning from radio to gamma rays. While MBHs accreting at significant fractions of their Eddington rate are readily detectable, those accreting at ...
Valentina La Torre, Fabio Pacucci
doaj   +1 more source

From Young Massive Clusters to Old Globular Clusters: Density Profile Evolution and Intermediate-mass Black Hole Formation

open access: yesThe Astrophysical Journal
The surface brightness profiles of globular clusters are conventionally described with the well-known King profile. However, observations of young massive clusters (YMCs) in the local Universe suggest that they are better fit by simple models with flat ...
Kuldeep Sharma, Carl L. Rodriguez
doaj   +1 more source

Interpretable machine learning for finding intermediate-mass black holes [PDF]

open access: green, 2023
Mario Pasquato   +6 more
openalex   +1 more source

Counting the Unseen. II. Tidal Disruption Event Rates in Nearby Galaxies with REPTiDE

open access: yesThe Astrophysical Journal
Tidal disruption events (TDEs) are a class of transients that occur when a star is destroyed by the tides of a massive black hole (MBH). Their rates encode valuable MBH demographic information, but this can only be extracted if accurate TDE rate ...
Christian H. Hannah   +3 more
doaj   +1 more source

Rates of Stellar Tidal Disruption Events around Intermediate-mass Black Holes

open access: yesThe Astrophysical Journal Letters
Rates of stellar tidal disruption events (TDEs) around supermassive black holes (SMBHs) have been extensively calculated using the loss cone theory, while theoretical work on TDE rates around intermediate-mass black holes (IMBHs) has been lacking.
Janet N. Y. Chang   +4 more
doaj   +1 more source

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