Two-temperature accretion around rotating black holes: a description of the general advective flow paradigm in the presence of various cooling processes to explain low to high luminous sources-Reference-Cited by-同舟云学术

Two-temperature accretion around rotating black holes: a description of the general advective flow paradigm in the presence of various cooling processes to explain low to high luminous sources

Published:2010-02-21 Issue:2 Volume:402 Page:961-984
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Rajesh S. R.,Mukhopadhyay Banibrata

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/402/2/961/3851042/mnras0402-0961.pdf

Reference54 articles.

1. Slim accretion disks

2. Thermal equilibria of accretion disks

3. Black holes in radiation-dominated gas: an analogue of the Bondi accretion problem

4. Thermal coupling of ions and electrons by collective effects in two-temperature accretion flows

5. The nature of SS433 and the ultraluminous X-ray sources

Cited by 44 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. A model on transition between steady states of sub-Keplerian accretion discs: implication for spectral states and hot corona above the disc;Astrophysics and Space Science;2024-05

2. Accretion flow in deformed Kerr spacetime: spectral energy distributions from free-free emission;Journal of Cosmology and Astroparticle Physics;2024-01-01

3. Thermal Conduction and Hydrodynamical Winds in Magnetized Viscous Accretion Disk Dynamics;2024

4. Magnetized Advective Accretion Disks and Jets: Harmpi Simulation;Astronomy Reports;2023-12

5. QPOs in Compact Sources as a Nonlinear Hydrodynamical Resonance: Determining Spin of Compact Objects;The Astrophysical Journal;2023-09-21