Star formation and the nature of bipolar outflows

Details Star formation and the nature of bipolar outflows Star formation and the nature of bipolar outflows

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370l..31s&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 370, March 20, 1991, p. L31-L34. Research supported by NSF and NA

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Molecular Clouds, Molecular Flow, Star Formation, Carbon Monoxide, Computational Astrophysics, Dynamic Models, Stellar Envelopes, Stellar Winds

Scientific paper

This paper presents a simple physical model for the bipolar molecular
outflows that frequently accompany star formation. The model forges an
intrinsic link between the bipolar flow phenomenon and the process of
star formation, and it helps to explain many of the systematics known
for existing sources.

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