Abstract
This article reviews recent studies of dynamics of disk-shaped galaxies with special emphasis on their spiral structures. In a local version of kinetic stability theory, the very existence and the value of the critical wavelength of the spiral structure arising due to nonresonant Jeans-type instability of gravity perturbations is explained. A formal analogy between the collective oscillations in a rotating self-gravitating disk and the oscillations of a hot nonneutral plasma in a magnetic field is explored.
Original language | English |
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Pages (from-to) | 47-56 |
Number of pages | 10 |
Journal | Advances in Space Research |
Volume | 38 |
Issue number | 1 |
DOIs | |
State | Published - 1 Jan 2006 |
Keywords
- Galaxies: Kinematics and dynamics
- Galaxies: Spiral galaxies
- Galaxies: Structure
- Waves and instabilities
ASJC Scopus subject areas
- Aerospace Engineering
- Astronomy and Astrophysics
- Geophysics
- Atmospheric Science
- Space and Planetary Science
- General Earth and Planetary Sciences