A fully relativistic twisted disc around a slowly rotating Kerr black hole: derivation of dynamical equations and the shape of stationary configurations-Reference-Cited by-同舟云学术

A fully relativistic twisted disc around a slowly rotating Kerr black hole: derivation of dynamical equations and the shape of stationary configurations

Published:2011-07-18 Issue:3 Volume:415 Page:2122-2144
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Zhuravlev V. V.,Ivanov P. B.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/415/3/2122/5968910/mnras0415-2122.pdf

Reference35 articles.

1. Radiation from relativistic particles in nongeodesic motion in a strong gravitational field

2. The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes

3. On X-ray emission lines from active galactic nuclei and disk models

4. Observational Evidence of Spin-induced Precession in Active Galactic Nuclei

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