This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

The Shakura-Sunyaev Disk Can Smoothly Match an Advection-dominated Accretion Flow

, , and

Published 2004 February 2 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Ju-Fu Lu et al 2004 ApJ 602 L37 DOI 10.1086/382209

1538-4357/602/1/L37

Abstract

We use the standard Runge-Kutta method to solve a set of basic equations describing black hole accretion flows composed of two-temperature plasma. We do not invoke any extra energy transport mechanism, such as thermal conduction, and we do not specify any ad hoc outer boundary condition for the advection-dominated accretion flow (ADAF) solution. We find that in the case of high viscosity and nonzero radiative cooling, the ADAF solution can have an asymptotic approach to the Shakura-Sunyaev disk (SSD) solution and that the SSD-ADAF transition radius is close to the central black hole. Our results further prove the mechanism of thermal instability-triggered SSD-ADAF transition suggested previously by Takeuchi & Mineshige and Gu & Lu.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/382209