Results 31 to 40 of about 8,250 (145)
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
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
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
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]
Jillian Bellovary +9 more
openalex +1 more source
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
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]
Mario Pasquato +6 more
openalex +1 more source
Counting the Unseen. II. Tidal Disruption Event Rates in Nearby Galaxies with REPTiDE
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
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

