A tidal disruption event from an intermediate-mass black hole revealed by comprehensive multi-wavelength observations [PDF]
Tidal disruption events (TDEs) occur when a star crosses the tidal radius of a black hole (BH) and is ripped apart, providing a powerful way to probe dormant BHs over a wide mass range.
Jialai Wang +14 more
doaj +2 more sources
Weighing the black holes in ultraluminous X-ray sources through timing [PDF]
We describe a new method to estimate the mass of black holes in Ultraluminous X-ray Sources (ULXs). The method is based on the recently discovered ``variability plane'', populated by Galactic stellar-mass black-hole candidates (BHCs) and supermassive ...
Belloni, T. +5 more
core +16 more sources
Partial Tidal Disruptions of Main-sequence Stars by Intermediate-mass Black Holes
We study close encounters of a 1 M _⊙ middle-age main-sequence star (modeled using MESA) with massive black holes through hydrodynamic simulations, and explore in particular the dependence of the outcomes on the black hole mass.
Fulya Kıroğlu +5 more
doaj +1 more source
Constraining a Companion of the Galactic Center Black Hole Sgr A*
We use 23 yr of astrometric and radial velocity data on the orbit of the star S0-2 to constrain a hypothetical intermediate-mass black hole orbiting the massive black hole Sgr A* at the Galactic center.
Clifford M. Will +6 more
doaj +1 more source
Multi-Messenger Astrophysics of a Millisecond Pulsar Orbiting around a Massive Black Hole
Extreme-mass-ratio and intermediate-mass-ratio binaries with a millisecond pulsar are gravitational-wave sources that emit also electromagnetic radiation.
Kinwah Wu
doaj +1 more source
Semiclassical S $$ \mathcal{S} $$ -matrix and black hole entropy in dilaton gravity
We use complex semiclassical method to compute scattering amplitudes of a point particle in dilaton gravity with a boundary. This model has nonzero minimal black hole mass M cr . We find that at energies below M cr the particle trivially scatters off the
Maxim Fitkevich +2 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
Investigating the mass of the intermediate mass black hole candidate HLX-1 with the SLIMBH model [PDF]
In this paper we present a comprehensive study of the mass of the intermediate mass black hole candidate HLX-1 in the galaxy ESO 243-49. We analyse the continuum X-ray spectra collected by Swift, XMM-Newton, and Chandra with the slim disc model, SLIMBH ...
Barret, Didier +4 more
core +4 more sources
Soap Bubbles in Outer Space: Interaction of a Domain Wall with a Black Hole [PDF]
We discuss the generalized Plateau problem in the 3+1 dimensional Schwarzschild background. This represents the physical situation, which could for instance have appeared in the early universe, where a cosmic membrane (thin domain wall) is located near a
A. L. Larsen +20 more
core +3 more sources
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

