Detection of the CO (J = 7 = 6) rotational transition at lambda = 0.37 millimeters toward Orion

Details Detection of the CO (J = 7 = 6) rotational transition at lambda = 0.37 millimeters toward Orion Detection of the CO (J = 7 = 6) rotational transition at lambda = 0.37 millimeters toward Orion

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...291l..59s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 291, April 15, 1985, p. L59-L61. Sponsorship: Deuts

Astronomy and Astrophysics

Astronomy

17

Astronomical Spectroscopy, Carbon Monoxide, Infrared Astronomy, Interstellar Gas, Molecular Rotation, Orion Nebula, Emission Spectra, Spectral Line Width, Submillimeter Waves

Scientific paper

The J = 7→6 rotational transition of carbon monoxide has been detected toward the Kleinmann-Low nebula. The peak antenna temperature is 110±35K centered at VLSR = +5 km s-1; the FWHM line width is 35±5 km s-1, and its optical depth ≤0.3. The integrated intensity of the line between -20 and +30 km s-1 leads to a total flux density of (2.5±0.5)×10-14W m-2 in the beam of 35arcsec±5arcsec.

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