Star formation and the nature of bipolar outflows

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 source...

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Veröffentlicht in:	The Astrophysical journal 1991-03, Vol.370 (1), p.L31-L34
Hauptverfasser:	Shu, Frank H., Ruden, Steven P., Lada, Charles J., Lizano, Susana
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources Astronomy ASTROPHYSICS CARBON COMPOUNDS CARBON MONOXIDE CARBON OXIDES CHALCOGENIDES CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC GASES Earth, ocean, space Exact sciences and technology FLUID FLOW FLUIDS Fundamental aspects of astrophysics Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations GAS FLOW GASES Hydrodynamics MATHEMATICAL MODELS MOLECULES OXIDES OXYGEN COMPOUNDS PROTOSTARS STAR EVOLUTION STAR MODELS STELLAR ACTIVITY STELLAR WINDS
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Beschreibung
Zusammenfassung:	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.
ISSN:	0004-637X 1538-4357
DOI:	10.1086/185970