Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...311.1073k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 311, Dec. 15, 1986, p. 1073-1075.
Astronomy and Astrophysics
Astrophysics
17
Interstellar Matter, Methyl Alcohol, Microwave Spectra, Molecular Rotation, Milky Way Galaxy
Scientific paper
Laboratory frequencies of 13CH3OH for all the rotational transitions with J ≤ 31, |k| ≤ 6, and υt = 0 in the 9 - 96 GHz region are reported, where υt is the quantum number for torsional vibrational state. The frequencies of the a-type, J = 1<-0 and 2<-1 transitions for υt = 1 and 2, and several b-type transitions for υt = 1 are also reported. The U line at 84970 MHz found in a spectral scan of Ori A by Johansson et al. is identified as the 808 - 717(A), υt = 0 transition of 13CH3OH.
Kuriyama Hirotada
Matsumura Chi
Takagi Kojiro
Takeo Harutoshi
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