
An asymptotic treatment of thin accretion disks, introduced by Klu��niak & Kita (2000) for a steady-state disk flow, is extended to a time-dependent problem. Transient growth of axisymmetric disturbances is analytically shown to occur on the global disk scale. The implications of this result on the theory of hydrodynamical thin accretion disks, as well as future prospects, are discussed.
To appear in New Astronomy Review, Proc. of "J-P. Lasota, X-ray binaries, accretion disks and compact stars" (October 2007); Abramowicz, M. Ed
Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics
Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics
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