Published September 1, 1987 | Version v1
Journal article

Physics of modes in a differentially rotating system -analysis of the shearing sheet

  • 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