Results 1 to 10 of about 63,717 (334)

Mergers of accreting stellar-mass black holes [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2016
We present post-Newtonian $N$-body simulations on mergers of accreting stellar-mass black holes (BHs), where such general relativistic effects as the pericenter shift and gravitational wave (GW) emission are taken into consideration.
Gouda, Naoteru   +2 more
core   +5 more sources

The Mass Distribution of Stellar-Mass Black Holes [PDF]

open access: yesThe Astrophysical Journal, 2010
We perform a Bayesian analysis of the mass distribution of stellar-mass black holes using the observed masses of 15 low-mass X-ray binary systems undergoing Roche lobe overflow and five high-mass, wind-fed X-ray binary systems.
Abadie   +33 more
core   +5 more sources

Impact of the Accretion Disk Thickness on the Polarization of the Thermal Emission from Stellar Mass Black Holes [PDF]

open access: goldThe Astrophysical Journal, 2023
The Imaging X-ray Polarimetry Explorer, launched in 2021 December, enables precision measurements of the energy-dependent polarization of the X-ray emission from stellar mass and supermassive black holes.
Andrew Thomas West, Henric Krawczynski
doaj   +2 more sources

Merging stellar-mass binary black holes [PDF]

open access: yesPhysics Reports, 2022
The LIGO and Virgo detectors have directly observed gravitational waves from mergers of pairs of stellar-mass black holes, along with a smaller number of mergers involving neutron stars. These observations raise the hope that compact object mergers could be used as a probe of stellar and binary evolution, and perhaps of stellar dynamics.
Ilya Mandel
exaly   +3 more sources

Mass Measurements of Stellar and Intermediate-Mass Black Holes [PDF]

open access: yesSpace Science Reviews, 2013
28 pages, 12 figures. Accepted for publication in Space Science Reviews (DOI 10.1007/s11214-013-0030-6). Also to appear in hard cover in the Space Sciences Series of ISSI "The Physics of Accretion onto Black Holes" (Springer Publisher).
Jorge Casares, Peter G Jonker
exaly   +7 more sources

Stellar‐Mass Black Holes in the Solar Neighborhood [PDF]

open access: bronzeThe Astrophysical Journal, 2003
We search for nearby, isolated, accreting, ``stellar-mass'' (3 to $100M_\odot$) black holes. Models suggest a synchrotron spectrum in visible wavelengths and some emission in X-ray wavelengths. Of 3.7 million objects in the Sloan Digital Sky Survey Early Data Release, about 150,000 objects have colors and properties consistent with such a spectrum, and
James R. Chisholm   +2 more
openalex   +4 more sources

The High Energy X-ray Probe (HEX-P): probing accretion onto stellar mass black holes [PDF]

open access: goldFrontiers in Astronomy and Space Sciences
Accretion is a universal astrophysical process that plays a key role in cosmic history, from the epoch of reionization to galaxy and stellar formation and evolution. Accreting stellar-mass black holes in X-ray binaries are one of the best laboratories to
Riley M. T. Connors   +24 more
doaj   +2 more sources

Templates for stellar mass black holes falling into supermassive black holes [PDF]

open access: yesClassical and Quantum Gravity, 2003
The spin modulated gravitational wave signals, which we shall call smirches, emitted by stellar mass black holes tumbling and inspiralling into massive black holes have extremely complicated shapes. Tracking these signals with the aid of pattern matching
Apostolatos T A   +7 more
core   +6 more sources

Stellar-Mass Black Holes and Ultraluminous X-ray Sources [PDF]

open access: yesScience, 2012
We review the likely population, observational properties, and broad implications of stellar-mass black holes and ultraluminous x-ray sources. We focus on the clear empirical rules connecting accretion and outflow that have been established for stellar-mass black holes in binary systems in the past decade and a half.
Rob Fender, Tomaso M Belloni
exaly   +4 more sources

Quasi-periodic oscillations of GHz-band polarization in a black hole [PDF]

open access: yesNature Communications
Relativistic jets from accreting black holes radiate non-thermal emission which is highly variable in different time scales. Previous studies on black holes of different mass scales, including supermassive and stellar-mass black holes, only report flux ...
Wei Wang   +12 more
doaj   +2 more sources

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