A highly collimated bipolar outflow in the core of OMC-1: CO submillimeter emission

Details A highly collimated bipolar outflow in the core of OMC-1: CO submillimeter emission A highly collimated bipolar outflow in the core of OMC-1: CO submillimeter emission

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..193s&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 193-195 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

1

Carbon Monoxide, Line Spectra, Molecular Clouds, Molecular Flow, Orion Nebula, Photodissociation, Spectral Emission, Submillimeter Waves, Bipolarity, Collimation, H Ii Regions

Scientific paper

A CO 7-6 survey of Orion Molecular Cloud (OMC)-1 reveals line wings, indicative of molecular outflow, at a position approximately two degrees south of the plateau/hot core source. A large bipolar flow system was found that displays the possibility that the lobe of blueshifted velocities protrude into the core of the H II region M42. Such a configuration permits studies of photodissociative interactions that develop and increase as the molecular jet approaches the ionized region. Large beam observations of the outflow region in higher CO transitions indicate the existence of line wings that might be the result of such interactions.

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