Results 31 to 40 of about 63,717 (334)
Kretschmann Scalar for a Kerr-Newman Black Hole [PDF]
I have derived the Kretschmann scalar for a general black hole of mass m, angular momentum per unit mass a, and electric charge Q. The Kretschmann scalar gives the amount of curvature of spacetime, as a function of position near (and within) a black hole.
Henry, Richard C.
core +3 more sources
An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing* [PDF]
Abstract We report the first unambiguous detection and mass measurement of an isolated stellar-mass black hole (BH). We used the Hubble Space Telescope (HST) to carry out precise astrometry of the source star of the long-duration (t E ≃ 270 days), high-magnification microlensing event MOA-2011-BLG-191/OGLE-2011-BLG-0462
Sahu, KC +194 more
openaire +13 more sources
The effect of stellar-mass black holes on the central kinematics of omega Cen: a cautionary tale for IMBH interpretations [PDF]
The search for intermediate-mass black holes (IMBHs) in the centre of globular clusters is often based on the observation of a central cusp in the surface brightness profile and a rise towards the centre in the velocity dispersion profiles.
Gieles, Mark +2 more
core +4 more sources
Gravitational Microlensing Events Due to Stellar‐Mass Black Holes [PDF]
We present an analysis of the longest timescale microlensing events discovered by the MACHO Collaboration during a 7 year survey of the Galactic bulge. We find 6 events that exhibit very strong microlensing parallax signals due, in part, to accurate photometric data from the GMAN and MPS collaborations. The microlensing parallax fit parameters are used
Bennett, D P +30 more
openaire +4 more sources
Observations have found black holes spanning 10 orders of magnitude in mass across most of cosmic history. The Kerr black hole solution is, however, provisional as its behavior at infinity is incompatible with an expanding universe.
Duncan Farrah +18 more
doaj +1 more source
Estimating the spins of stellar-mass black holes [PDF]
We describe a program that we have embarked on to estimate the spins of stellar-mass black holes in X-ray binaries. We fit the continuum X-ray spectrum of the radiation from the accretion disk using the standard thin disk model, and extract the dimensionless spin parameter a* = a/M of the black hole as a parameter of the fit.
McClintock, Jeffrey E. +2 more
openaire +2 more sources
Black holes in stellar-mass binary systems: expiating original spin? [PDF]
Accepted for publication in MNRAS in original form.
King, A., Nixon, C.
openaire +3 more sources
By using direct N -body numerical simulations, we model the dynamical coevolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to investigate how different stellar components evolve during the merger, we
Shuo Li +5 more
doaj +1 more source
We study radio and X-ray emissions from intermediate-mass black holes (IMBHs) and explore the unified model for accretion and ejection processes. The radio band survey of IMBH (candidate) hosted galaxies indicates that only a small fraction (∼0.6%) of ...
Xiaolong Yang, Jun Yang
doaj +1 more source
The Dynamical Evolution of Stellar Black Holes in Globular Clusters
Our current understanding of the stellar initial mass function and massive star evolution suggests that young globular clusters may have formed hundreds to thousands of stellar-mass black holes, the remnants of stars with initial masses from $\sim 20 ...
Morscher, Meagan +4 more
core +1 more source

