A note on the conditions for SSD-ADAF transitions

Details A note on the conditions for SSD-ADAF transitions A note on the conditions for SSD-ADAF transitions

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.293..443a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 293, p. 443

Astronomy and Astrophysics

Astronomy

28

Accretion Disks, Hydrodynamics, Astronomical Models, Kepler Laws, Orbital Velocity

Scientific paper

One of the necessary matching conditions between an optically thin, hot, advectively dominated part of an accretion disk (ADAF) and the standard Shakura-Sunyaev disk (SSD) part is that the matching transition region must rotate with an orbital speed that is faster than the Keplerian one. We discuss properties of the SSD-ADAF transition in terms of a simple two-dimensional hydrodynamical model.

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