Oscillations in star formation and contents of a molecular cloud complex

Details Oscillations in star formation and contents of a molecular cloud complex Oscillations in star formation and contents of a molecular cloud complex

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...142..297b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 142, no. 2, Jan. 1985, p. 297-315. Research supported by the Nationaal Fonds v

Astronomy and Astrophysics

Astrophysics

21

Interstellar Matter, Molecular Clouds, Star Formation, Stellar Oscillations, Early Stars, H Ii Regions, Milky Way Galaxy, Negative Feedback, Positive Feedback

Scientific paper

The present investigation is concerned with a model of a star-forming region with negative and positive feedback mechanisms. The three components of the model include cool H I gas, dusty molecular gas, and young stars with their associated H II regions. Attention is given to star formation and the interstellar medium (ISM), stellar evolution with mass loss, the synthesis of molecules, aspects of numerical analysis, and observational evidence. It is shown that star formation can be controlled by positive feedback mechanisms as a consequence of the intrinsic instability of gravitationally driven cloud processes and the interaction of young stars with the interstellar medium.

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