A review of quasi-periodic oscillations from black hole X-ray binaries: Observation and theory
Adam Ingram,Sara Motta +1 more
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In this paper, the authors review the basic phenomenology of different varieties of quasi-periodic oscillations (QPOs) in both black hole and neutron star X-ray binary systems and focus mainly on low frequency QPOs in black hole systems.About:
This article is published in New Astronomy Reviews.The article was published on 2019-09-01 and is currently open access. It has received 114 citations till now. The article focuses on the topics: Black hole & Nodal precession.read more
Citations
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Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
Roy P. Kerr,Roy P. Kerr +1 more
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Black holes in binary systems
TL;DR: A detailed view of the possible detection of a black hole can be found in this article, where the authors show a schematic view of a path leading to this objective from observations of existing type.
Journal Article
A 400 solar mass black hole in the galaxy M82
TL;DR: Stable, twin-peak (3:2 frequency ratio) X-ray quasi-periodic oscillations from M82 X-1 are reported and the black hole mass is estimated to be 428 ± 105 solar masses using the relativistic precession model.
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The Distance, Inclination, and Spin of the Black Hole Microquasar H1743-322
TL;DR: In this paper, a simple and symmetric kinematic model was applied to the trajectories of two-sided radio and X-ray jets of H1743-322 to determine the source distance, 8.5 \pm 0.8 kpc and inclination angle of the jets, 75 \pm 3 degrees.
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Neutron stars and the nuclear equation of state
TL;DR: In this paper, the authors review the current status and recent progress of microscopic many-body approaches and phenomenological models, which are employed to construct the equation of state of neutron stars.
References
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A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
Steven A. Balbus,John F. Hawley +1 more
TL;DR: In this article, a linear analysis is presented of the instability, which is local and extremely powerful; the maximum growth rate which is of the order of the angular rotation velocity, is independent of the strength of the magnetic field.
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Gravitational field of a spinning mass as an example of algebraically special metrics
Roy P. Kerr,Roy P. Kerr +1 more
Journal ArticleDOI
X-Ray Properties of Black-Hole Binaries
TL;DR: In this paper, the authors review the properties and behavior of 20 X-ray binaries that contain a dynamically confirmed black hole, 17 of which are transient systems, during the past decade, many of these transien...
Journal ArticleDOI
Rotating Black Holes: Locally Nonrotating Frames, Energy Extraction, and Scalar Synchrotron Radiation
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Black holes in binary systems. Observational appearance
N. I. Shakura,R. A. Sunyaev +1 more
TL;DR: In this paper, the structure and radiation spectrum of the disk around a black hole are investigated. But the authors focus on the formation of a disk around the black hole and not on the physical structure of the accreting matter.