Viscosity prescriptions in accretion discs with shock waves
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1995-01-01 and is currently open access. It has received 76 citations till now. The article focuses on the topics: Accretion (astrophysics).read more
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Zero-Energy Rotating Accretion Flows near a Black Hole
TL;DR: In this paper, the authors characterize the nature of thin, axisymmetric, inviscid accretion flows of cold adiabatic gas with zero specific energy in the vicinity of a black hole by the specific angular momentum.
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Line Emission from an Accretion Disk around a Rotating Black Hole: Toward a Measurement of Frame Dragging
TL;DR: Tanaka et al. as mentioned in this paper showed that the first three moments of a line profile define a three-dimensional space in which the presence of material at small radii becomes quantitatively evident in broad classes of disk models.
Journal ArticleDOI
Spectral Properties of Accretion Disks around Black Holes. II. Sub-Keplerian Flows with and without Shocks
TL;DR: In this paper, the spectral properties of various models of accretion disks in which a Keplerian disk on the equatorial plane may or may not be flanked by a sub-Keplerian disk and the sub-keplerian flow may not possess standing shocks were studied.
Journal ArticleDOI
Zero Energy Rotating Accretion Flows near a Black Hole
TL;DR: In this paper, the authors characterize the nature of thin, axisymmetric, inviscid, accretion flows of cold adiabatic gas with zero specific energy in the vicinity of a black hole by the specific angular momentum.