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
Relativistic Collapse of Rotating Supermassive Stars to Supermassive Black Holes
There is compelling evidence that supermassive black holes (SMBHs) exist. Yet the origin of these objects, or their seeds, is still unknown. We are performing general relativistic simulations of gravitational collapse to black holes in different ...
Shapiro, Stuart L.
core +2 more sources
Gravitational lensing effects of supermassive black holes in cluster environments [PDF]
Guillaume Mahler +3 more
openalex +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
High Proper‐Motion Stars in the Vicinity of Sagittarius A*: Evidence for a Supermassive Black Hole at the Center of Our Galaxy [PDF]
A. M. Ghez +3 more
openalex +1 more source
Towards measuring supermassive black hole masses with interferometric\n observations of the dust continuum [PDF]
A. Amorim +41 more
openalex +1 more source
Bayesian Black Hole Photogrammetry
We propose an analytic dual-cone accretion model for horizon-scale images of the cores of low-luminosity active galactic nuclei, including those observed by the Event Horizon Telescope (EHT).
Dominic O. Chang +3 more
doaj +1 more source
Evolution of supermassive stars as a pathway to black hole formation
Supermassive stars, with masses greater than a million solar masses, are possible progenitors of supermassive black holes in galactic nuclei. Because of their short nuclear burning timescales, such objects can be formed only when matter is able to ...
Begelman +29 more
core +1 more source
CONSTRAINING SUB-PARSEC BINARY SUPERMASSIVE BLACK HOLES IN QUASARS WITH MULTI-EPOCH SPECTROSCOPY. II. THE POPULATION WITH KINEMATICALLY OFFSET BROAD BALMER EMISSION LINES [PDF]
Xin Liu +4 more
openalex +1 more source
Emission Signatures from Subparsec Binary Supermassive Black Holes. III. Comparison of Models with Observations [PDF]
Khai Nguyen +5 more
openalex +1 more source

