Structure Formation in Anisotropic Disks
2006 ◽
Vol 2
(S235)
◽
pp. 143-143
Keyword(s):
The majority of normal disk galaxies are characterized by non-axisymmetric structures like spirals or bars. These structural elements have been widely discussed in the literature as a result of gravitational instabilities which are connected to growing density waves or global instabilities of disks. A first insight into the properties of galactic discs was provided by linear stability analysis. However, a disadvantage of linear stability analysis remained its restriction to small perturbations, both in amplitude and wavelength. Thus, numerical simulations, especially hydrodynamical and stellar-hydrodynamical simulations became a primary tool for the analysis of galactic evolution.
Keyword(s):
Keyword(s):
2021 ◽
Vol 198
◽
pp. 106392