Accretion Disk Boundary Layers - Their Structure and Stability

Details Accretion Disk Boundary Layers - Their Structure and Stability Accretion Disk Boundary Layers - Their Structure and Stability

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..315s&link_type=abstract

Astrophysics and Space Science, Volume 130, Issue 1-2, pp. 315-320

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The importance of the boundary layer has been known for some time, (see Lynden-Bell and Pringle, 1974). Yet this region of the disc has never been studied in great depth. The authors present here some calculations which are undertaken in order to explore some of the complex processes which can go on in this region. It is shown how the structure of the boundary layer is affected by viscosity, how oscillations can occur in the outer disk and boundary layer regions. The authors also show how they disperse and dissipate.

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