Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..249w&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 1, p. 249-254.
Astronomy and Astrophysics
Astrophysics
12
Electron Transitions, Emission Spectra, Interstellar Matter, Masers, Methyl Alcohol, Astronomical Spectroscopy, Interstellar Chemistry, Molecular Excitation
Scientific paper
Measurements of the J(k) = 13(2) - 13(1)E (27.471 GHz), the 4(0) - 3(1)E (28.316GHz) and the 8(2) - 9(1)A (28.970GHz) lines of CH3OH with the 100-m telescope are reported; the 13(2) - 13(1)E and 8(2) - 9(1)A- lines have been found for the first time in astronomical sources. The 8(2) - 9(1)A- line is found in emission toward the compact HII region W3 (OH). Presumably this line is produced by maser action. The 4(0) - 3(1)E line is found in absorption. Toward Orion KL, these three lines appear as two blended emission features. The most intense feature is centered between 5 and 10 arcsec south of the Hot Core region. The sizes range from less than 15 to 20 arcsec. The rotational temperature obtained from these results is 100 K, somewhat lower than previously obtained. Weak emission from W51 el/e2 in the 4(0) - 3(1)E line was also detected. For W3 (OH) and Orion KL, the column densities obtained from measurements of the 4(0) - 3(1)E lines exceed the predicted values by more than a factor of two. The excitation of these methanol lines is discussed.
Dahmen G.
Henkel Carsten
Huettemeister Susanne
Wilson Thomas L.
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