An exact solution for an isothermal gas cloud with fast differential rotation

Details An exact solution for an isothermal gas cloud with fast differential rotation An exact solution for an isothermal gas cloud with fast differential rotation

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120..234s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 2, April 1983, p. 234-236.

Astronomy and Astrophysics

Astrophysics

12

Galactic Structure, Protostars, Rotating Matter, Differential Equations, Mathematical Models

Scientific paper

Properties of an isothermal self-gravitating gas cloud with fast differential rotation, infinite extension, a flattened density distribution, and finite central density are discussed. It is described by a simple exact solution of the equations of structure of self-gravitating and rotating gaseous masses. These are transformed to a simple differential equation which seems appropriate for search of exact solutions. Further attempts to find other exact solutions are discussed.

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