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Advective accretion disks and related problems including magnetic fields
Accretion disk theory was first developed assuming local heat balance where the energy
produced by viscous heating was emitted from the sides of the disk. One of the important …
produced by viscous heating was emitted from the sides of the disk. One of the important …
Supercritical accretion flows around black holes: two-dimensional, radiation pressure-dominated disks with photon trap**
K Ohsuga, M Mori, T Nakamoto… - The Astrophysical …, 2005 - iopscience.iop.org
The quasi-steady structure of supercritical accretion flows around a black hole is studied
based on two-dimensional radiation-hydrodynamic (2D-RHD) simulations. The supercritical …
based on two-dimensional radiation-hydrodynamic (2D-RHD) simulations. The supercritical …
Zero-energy rotating accretion flows near a black hole
We 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 …
gas with zero specific energy in the vicinity of a black hole by the specific angular …
Viscous accretion discs around rotating black holes
J Peitz, S Appl - Monthly Notices of the Royal Astronomical …, 1997 - academic.oup.com
The stationary hydrodynamic equations for transonic viscous accretion discs in Kerr
geometry are derived. A consistent formulation is given for the viscous angular momentum …
geometry are derived. A consistent formulation is given for the viscous angular momentum …
Rotating accretion flows: From infinity to the black hole
Accretion onto a supermassive black hole of a rotating inflow is a particularly difficult
problem to study because of the wide range of length scales involved. There have been …
problem to study because of the wide range of length scales involved. There have been …
Spectral properties of accretion disks around black holes. II. Sub-Keplerian flows with and without shocks
Close to a black hole, the density of the sub-Keplerian accreting matter becomes higher
compared with a spherical flow as a consequence of the presence of a centrifugal barrier …
compared with a spherical flow as a consequence of the presence of a centrifugal barrier …
Influence of ohmic heating on advection-dominated accretion flows
Abstract Advection-dominated, high-temperature, quasi-spherical accretion flow onto a
compact object, recently considered by a number of authors, assumes that the dissipation of …
compact object, recently considered by a number of authors, assumes that the dissipation of …
Estimation of mass of compact object in H 1743-322 from 2010 and 2011 outbursts using TCAF solution and spectral index–QPO frequency correlation
The well-known black hole candidate (BHC) H 1743-322 exhibited temporal and spectral
variabilities during several outbursts. The variation of the accretion rates and flow geometry …
variabilities during several outbursts. The variation of the accretion rates and flow geometry …
Accretion flow dynamics of MAXI J1836-194 during its 2011 outburst from TCAF solution
The Galactic transient X-ray binary MAXI J1836-194 was discovered on 2011 August 29.
Here we make a detailed study of the spectral and timing properties of its 2011 outburst …
Here we make a detailed study of the spectral and timing properties of its 2011 outburst …
Properties of accretion shock waves in viscous flows around black holes
Accretion flows having low angular momentum and low viscosity can have standing shock
waves. These shocks arise because of the presence of multiple sonic points in the flow. We …
waves. These shocks arise because of the presence of multiple sonic points in the flow. We …