Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...240..191s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 240, no. 1, Dec. 1990, p. 191-202.
Astronomy and Astrophysics
Astrophysics
17
Accretion Disks, Gravitational Effects, Hydrodynamics, Perturbation Theory, Angular Momentum, Conservation Laws, Density (Mass/Volume), Modal Response, Vorticity
Scientific paper
The linear stability of a thin differentially rotating gaseous disk with reflecting boundaries against nonaxisymmetric perturbations is considered. The relevant conservation laws for the energy and angular momentum of linear nonaxisymmetric modes in a thin rotating disk without self-gravity are discussed, and the basic mode amplification mechanisms are illustrated with numerical solutions. How the frequency and growth rate of unstable modes depend on the distribution of the ratio of vorticity to surface density in the disk is investigated.
Heemskerk M. H. M.
Savonije G. J.
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