Results 91 to 100 of about 34,507 (229)
We propose that modifications to the Higgs potential within a narrow atmospheric layer near the event horizon of an astrophysical black hole could significantly enhance the rate of sphaleron transitions, as well as transform the Chern–Simons number into ...
Merab Gogberashvili+1 more
doaj +1 more source
Two Radio Cores in GPS J1543-0757: A New Dual Supermassive Black Hole System?
We report on the discovery of a dual supermassive black hole system in the radio galaxy J1543−0757, with a projected separation between the two black holes of ∼46 mas. The result is based on recent multifrequency observations using the Very Long Baseline
Xiaopeng Cheng, Bong Won Sohn
doaj +1 more source
A population of luminous accreting black holes with hidden mergers
Major galaxy mergers are thought to play an important part in fuelling the growth of supermassive black holes. However, observational support for this hypothesis is mixed, with some studies showing a correlation between merging galaxies and luminous ...
A DasGupta+69 more
core +1 more source
Tidal disruption flares from stars on eccentric orbits
We study tidal disruption and subsequent mass fallback for stars approaching supermassive black holes on bound orbits, by performing three dimensional Smoothed Particle Hydrodynamics simulations with a pseudo-Newtonian potential.
Loeb A., Stone N., Hayasaki K.
doaj +1 more source
Soft gamma rays from low accreting supermassive black holes and connection to energetic neutrinos. [PDF]
Kimura SS, Murase K, Mészáros P.
europepmc +1 more source
We consider test planet and photon orbits of the third kind inside a black hole, which are stable, periodic and neither come out of the black hole nor terminate at the singularity.
B. Carter+6 more
core +1 more source
A Comparison of the X-Ray Polarimetric Properties of Stellar and Supermassive Black Holes
X-ray polarization provides a new way to probe accretion geometry in black hole systems. If the accretion geometry of black holes is similar regardless of mass, we should expect the same to be true of their polarization properties.
M. Lynne Saade+3 more
doaj +1 more source
Supermassive black holes at high redshifts [PDF]
MeV blazars are the most luminous persistent sources in the Universe and emit most of their energy in the MeV band. These objects display very large jet powers and accretion luminosities and are known to host black holes with a mass often exceeding $10^9
Agudo, Ivan+34 more
core +1 more source
26 pages, 15 figures, to appear in "Kerr Spacetime: Rotating Black Holes in General Relativity" eds. D.L. Wiltshire, M. Visser and S.M. Scott, (Cambridge Univ. Press)
openaire +2 more sources
The Millennium Galaxy Catalogue: The nearby supermassive black hole mass function
We highlight the correlation between a galaxy's supermassive black hole mass and the Sersic-index of the host spheroid or bulge component. From our bulge-disk decompositions of 10 095 galaxies, drawn from the Millennium Galaxy Catalogue, we construct the
Allen, Paul D.+3 more
core +2 more sources