C-13H3OH in OMC-1

Details C-13H3OH in OMC-1 C-13H3OH in OMC-1

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...286..586b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 286, Nov. 15, 1984, p. 586-590.

Astronomy and Astrophysics

Astrophysics

31

Astronomical Spectroscopy, Interstellar Matter, Methyl Alcohol, Molecular Clouds, Molecular Spectra, Acetaldehyde, Interstellar Chemistry, Line Spectra, Molecular Rotation

Scientific paper

Transition line data for C-13H3OH in OMC-1 were gathered with a superconducting tunnel junction receiver and a 512 channel spectrometer on a 10.4 m telescope at the Owens Valley Radio Observatory. The methanol was scanned at 236 GHz and an observational efficiency of 85 percent. The survey was carried out to complement the data base on the line frequencies of internal rotors such as methanol and thereby the resolution of the C-12/C-13 ratio toward the galactic center. The data indicated that previous emission lines attributed to CO(+) and CH3CHO are actually methanol emissions, and the associated C-12/C-13 ratio is about 30.

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