Methyl cyanide in Orion-KL

Details Methyl cyanide in Orion-KL Methyl cyanide in Orion-KL

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..705h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 2, Dec. 1991, p. 705-711.

Astronomy and Astrophysics

Astrophysics

4

Acetonitrile, Interstellar Matter, Molecular Clouds, Star Formation, Ammonia, Carbon Monoxide, Emission Spectra, Formaldehyde, Hydrogen, Masers, Stellar Composition, Temperature Distribution, Water

Scientific paper

Observations of 349 GHz J = 19-18 CH3CN in Orion-KL are reported. Two
velocity components have been detected, one corresponding with the
quiescent ridge and another with a more turbulent cloud. The latter is
centered 10 arcsec northeast of IRc2 and appears to be another site of
ongoing star formation and a source of bipolar outflow.

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