Evolution of interstellar clouds towards star formation. I - The density-mass diagram of polytropic models

Details Evolution of interstellar clouds towards star formation. I - The density-mass diagram of polytropic models Evolution of interstellar clouds towards star formation. I - The density-mass diagram of polytropic models

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13...35k&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, March 1989, p. 35-45. Translation.

Astronomy and Astrophysics

Astrophysics

Interstellar Matter, Mass Distribution, Molecular Clouds, Polytropic Processes, Star Formation, Chemical Composition, Gravitational Fields, Stellar Evolution

Scientific paper

The density-mass diagram in the study of the evolution of interstellar clouds is discussed. Three different forms of the diagram are noted. Using the polytrope model, the mean density, total mass, surface conditions (pressure and temperature) and the polytropic index are used as the main model parameters. The properties of the models under the critical state of gravitational instability and their behavior on the density-mass diagram are discussed.

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