Bipolar molecular outflows

Details Bipolar molecular outflows Bipolar molecular outflows

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26arv...3..257b&link_type=abstract

Astronomy and Astrophysics Review (ISSN 0935-4956), vol. 3, no. 3-4, April 1992, p. 257-287. Research supported by CICYT.

Astronomy and Astrophysics

Astronomy

81

Early Stars, Molecular Clouds, Radio Astronomy, Radio Jets (Astronomy), Star Formation, Carbon Monoxide, Interstellar Matter, Millimeter Waves, Stellar Cores, Stellar Evolution, Stellar Winds

Scientific paper

The main observational properties of the outflows around young stellar objects are reviewed highlighting recent information provided by large radiotelescopes operating at millimeter wavelengths (in particular the IRAM 30-m, the NRO 45-m, and the JCMT 15-m dishes). The observations of outflows containing molecular jet-like flows and 'bullets' are discussed in detail to provide key information for understanding the origin and evolution of the outflows. A number of closely related issues are examined including: the evidence for dense shocked gas associated with the flows; the interaction of the outflows with the ambient dense cores; the evolutionary status of the sources driving the outflows; the properties of circumstellar disks; and theoretical models of the origin of the neutral winds. All these areas are important for developing a plausible scenario for the formation and evolution of the bipolar molecular outflows.

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