CO/J = 6-5/ distribution in Orion and detection in other galactic sources

Details CO/J = 6-5/ distribution in Orion and detection in other galactic sources CO/J = 6-5/ distribution in Orion and detection in other galactic sources

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...260..584k&link_type=abstract

Astrophysical Journal, Part 1, vol. 260, Sept. 15, 1982, p. 584-589.

Other

38

Astronomical Spectroscopy, Carbon Monoxide, Interstellar Matter, Molecular Spectra, Orion Nebula, Calibrating, Emission Spectra, Infrared Telescopes, Line Shape, Molecular Clouds, Submillimeter Waves

Scientific paper

The profile of the CO line in Orion has been studied at 691 GHz with the NASA infrared telescope at Mauna Kea using a laser heterodyne receiver. The line from the BN/KL region is very broad and has a peak temperature of 180 K. Away from BN/KL, the emission line becomes narrow, and the intensity falls off rapidly. Several other galactic sources were also detected.

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