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Star formation and the nature of bipolar outflowsThis 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.
Document ID
19910042478
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/185970
Authors
Shu, Frank H. (California, University Berkeley, United States)
Ruden, Steven P. (California, University Irvine and Berkeley, United States)
Lada, Charles J. (Steward Observatory Tucson, AZ, United States)
Lizano, Susana (Universidad Nacional Autonoma de Mexico Mexico City, Mexico)
Date Acquired
August 14, 2013
Publication Date
March 20, 1991
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 370
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A27101
Distribution Limits
Public
Copyright
Other

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