Thermal Emission of Methanol and Other Molecules at Millimeter Wavelengths

Details Thermal Emission of Methanol and Other Molecules at Millimeter Wavelengths Thermal Emission of Methanol and Other Molecules at Millimeter Wavelengths

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46...96k&link_type=abstract

Astronomy Reports, Volume 46, Issue 2, February 2002, pp.96-109

Astronomy and Astrophysics

Astronomy

2

Scientific paper

The paper reports the results of a survey of Galactic star-forming regions in the methanol lines 8-1 70 E at 229.8 GHz, 3-2 4-1 E at 230.0 GHz, 00 1-1 E at 108.9 GHz, and a series of J 1 J 0 E lines near 165 GHz. In addition to the methanol lines, lines of methyl cyanide (CH3CN), cyanoacetylene (HC3N), methyl formate (HCOOCH3), and sulphur dioxide (SO2) were detected. Analysis of the data indicates that the methanol emission arises in warm (30 50 K) gas.

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