The locations of newly formed stars in molecular clouds

Details The locations of newly formed stars in molecular clouds The locations of newly formed stars in molecular clouds

Oct 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978m%26p....19..157l&link_type=abstract

(Conference on Protostars and Planets, Tucson, Ariz., Jan. 3-7, 1978.) Moon and the Planets, vol. 19, Oct. 1978, p. 157, 158.

Physics

1

B Stars, Gravitational Collapse, Hydrogen Clouds, Molecular Gases, O Stars, Protostars, Stellar Evolution, Cloud Physics, Fragmentation, Molecular Interactions, Stellar Mass

Scientific paper

Observations of very massive stars (at least 10 solar masses) are suggestive of a star formation process which requires an external trigger. However, observations pertaining to the formation of stars of lower mass (no more than 9 solar masses) require no such triggering mechanism and are consistent with the idea that such stars form as a natural consequence of the evolution, gravitational collapse, and fragmentation of a protostellar molecular cloud.

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