Transition from a Shakura-Sunyaev disk to an advection-dominated accretion flow

Details Transition from a Shakura-Sunyaev disk to an advection-dominated accretion flow Transition from a Shakura-Sunyaev disk to an advection-dominated accretion flow

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cha%26a..26....7p&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 26, Issue 1, p. 7-13.

Astronomy and Astrophysics

Astrophysics

2

Black Hole, Accretion Disk, Radiation Mechanism

Scientific paper

This paper studies the mechanism of transition from a Shakura-Sunyaev disk to an advection-dominated accretion flow in more details, taking into consideration two-temperature plasma accretion flows with bremsstrahlung and synchrotron radiation and Comptonization. The results further show that such a transition is realizable for a quite wide range of physical conditions.

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