Non-Uniformly Rotating, Self-Gravitating, Compressible Masses with Internal Meridian Circulation

Details Non-Uniformly Rotating, Self-Gravitating, Compressible Masses with Internal Meridian Circulation Non-Uniformly Rotating, Self-Gravitating, Compressible Masses with Internal Meridian Circulation

Apr 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..27..425r&link_type=abstract

Astrophysics and Space Science, Volume 27, Issue 2, pp.425-435

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

The structure of self-gravitating, inviscid, compressible fluids is
investigated assuming a polytropic relation between pressure and
density. A class of solutions with non-uniform rotation and internal
meridian circulation are presented and the stream lines of the flow
calculated using a perturbation technique.

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