Abstract
An improved linear stability theory of small-amplitude oscillations of a
self-gravitating, infinitesimally thin gaseous disk of spiral galaxies
has been developed. It was shown that in the differentially rotating
disks for nonaxisymmetric perturbations Toomre's modified hydrodynamical
simulations to test the validity of the modified local criterion.
Original language | English |
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Pages (from-to) | 131-134 |
Journal | Astronomical and Astrophysical Transactions |
Volume | 20 |
Issue number | 1 |
DOIs | |
State | Published - 1 Jun 2001 |