Results 41 to 50 of about 237,520 (386)
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
Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4−055108 [PDF]
We recently discovered the X-ray/optical outbursting source 3XMM J215022.4−055108. It was best explained as the tidal disruption of a star by an intermediate-mass black hole of mass of a few tens of thousand solar masses in a massive star cluster at the ...
D. Lin+8 more
semanticscholar +1 more source
X-ray spectroscopy of Galactic black hole binaries serves as a powerful tool to gain an overall understanding of the system. Not only can the properties of the accretion disk be studied in detail, the fundamental properties of the black hole such as spin
Sandeep K. Rout+3 more
doaj +1 more source
Intermediate mass black hole formation in compact young massive star clusters [PDF]
Young dense massive star clusters are a promising environment for the formation of intermediate mass black holes (IMBHs) through collisions. We present a set of 80 simulations carried out with Nbody6++GPU of 10 initial conditions for compact $\sim 7 ...
F. Rizzuto+15 more
semanticscholar +1 more source
Searching for intermediate-mass black holes in NGC3310 [PDF]
Six pages, two figures.
Megan Argo+4 more
openaire +3 more sources
Radio Emission from an Ultraluminous X-Ray Source [PDF]
The physical nature of ultraluminous x-ray sources is uncertain. Stellar mass black holes with beamed radiation and intermediate mass black holes with isotropic radiation are two plausible explanations.
Corbel, Stephane+3 more
core +3 more sources
The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center [PDF]
We report the results of high-resolution molecular line observations of the high-velocity compact cloud HCN–0.085–0.094 with the Atacama Large Millimeter/submillimeter Array. The HCN J = 4–3, HCO+ J = 4–3, and CS J = 7–6 line images reveal that HCN–0.085–
S. Takekawa+4 more
semanticscholar +1 more source
Looking for Intermediate-Mass Black Holes [PDF]
A discussion of the entropy of the universe leads to the suggestion of very many intermediate-mass black holes between thirty and three hundred thousand solar masses in the halo. It is consistent with observations on wide binaries as well as microlensing and considerations of disk stability that such IMBHs constitute all cold dark ...
openaire +4 more sources
Radio Detections During Two State Transitions of the Intermediate Mass Black Hole HLX-1 [PDF]
Relativistic jets are streams of plasma moving at appreciable fractions of the speed of light. They have been observed from stellar mass black holes ($\sim$3$-$20 solar masses, M$_\odot$) as well as supermassive black holes ($\sim$10$^6$$-$10$^9$ M$_ ...
Barret, Didier+9 more
core +6 more sources
Does NGC 6397 contain an intermediate-mass black hole or a more diffuse inner subcluster? [PDF]
We analyze proper motions from the Hubble Space Telescope (HST) and the second Gaia data release along with line-of-sight velocities from the MUSE spectrograph to detect imprints of an intermediate-mass black hole (IMBH) in the center of the nearby, core-
Eduardo Vitral, G. Mamon
semanticscholar +1 more source