Published September 1, 1987
| Version v1
Journal article
Physics of modes in a differentially rotating system -analysis of the shearing sheet
Creators
- 1. Steward Observatory, Tucson, AZ (USA)
- 2. California Inst. of Tech., Pasadena (USA)
- 3. Institute for Advanced Study, Princeton, NJ (USA)
Description
An analysis is given of the linear non-vortical modes of the shearing sheet, a model compressible two-dimensional fluid system with constant density, constant shear, and Coriolis force. This model has several features found in differentially rotating systems of interest in astrophysics, such as disc galaxies, accretion tori, planetary rings, protostellar nebulae, and possibly even rotating stars. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 228
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 1-41
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 19006870
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCRETION DISKS; CORIOLIS FORCE; FLUID FLOW; GALAXIES; MATHEMATICAL MODELS; NEBULAE; PROTOSTARS; ROTATION; SHEAR; TORI