Thin disk approximations and the equilibrium structure of polytropic disks

Details Thin disk approximations and the equilibrium structure of polytropic disks Thin disk approximations and the equilibrium structure of polytropic disks

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...230..509s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 230, no. 2, April 1990, p. 509-517.

Statistics

Computation

4

Equilibrium Equations, Gravitational Fields, Interstellar Matter, Polytropic Processes, Rotating Matter, Star Formation, Computational Astrophysics, Thin Bodies

Scientific paper

The equilibrium equations of rotating axially symmetric infinitely thin
disks with self-gravitation and a two-dimensional polytropic pressure
are studied. The structure of nonrotating polytropic disks is
calculated. It is shown that the structure of these disks behaves
similarly to that of corresponding spheres.

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