A new bipolar outflow source in OMC-1

Details A new bipolar outflow source in OMC-1 A new bipolar outflow source in OMC-1

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...356l..25z&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 356, June 10, 1990, p. L25-L29.

Astronomy and Astrophysics

Astrophysics

42

Bipolarity, Interstellar Gas, Orion Nebula, Star Formation, Stellar Winds, Early Stars, Molecular Clouds, Red Shift, Stellar Mass

Scientific paper

Observations of the J = 2-1 and J = 5-4 transitions of SiO have been made toward the outflow source about 1.5 arcmin south of Orion-KL, using the IRAM 30-m telescope, with 25- and 13-arcsec resolution, respectively. Additional measurements of the J = 2-1, 3-2, and 5-4 lines of C34S and observations of J = 5-4 and J = 13-12 transitions of CH3CN have been made with the 30-m telescope. The SiO data clearly indicate that a separate outflow source exists about 100 arcsec S and 20 arcsec W of the Orion-KL/IRc2 position.

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