Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...442..668s&link_type=abstract
Astrophysical Journal (ISSN 0004-637X), vol. 442, no. 2, Part 1, p. 668-673
Astronomy and Astrophysics
Astronomy
33
H Ii Regions, Interstellar Masers, Line Spectra, Methyl Alcohol, Millimeter Waves, Molecular Clouds, Radio Astronomy, Velocity Distribution, Astronomical Spectroscopy, Molecular Flow, Molecular Rotation, Shock Waves, Spectrum Analysis, Thermal Emission
Scientific paper
The series of methanol J0-J-1 E lines at 157 GHz has been detected in known methanol line sources together with the 21-30 A+ line of A-type methanol. In W3(OH), 345.01+1.79, W48, and Cep A the Jo-J-1 lines are intense and narrow and are believed to be maser lines. The radial velocities and profiles are similar to those of other class II methanol lines in these sources. The intensity of the lines increases with rotational number J, in contrast to thermal methanol features which were detected in the same sources at slightly different radial velocities. It is suggested that the new maser line sources are the class II methanol masers but are excited with higher radiation temperature than the lower frequency class II masers at 6.7 and 12.2 GHz. The masers may be related to molecular outflows or cometary bow shocks of ultracompact H II regions as is evidenced by their velocity shift relative to the parent molecular clouds.
Kalenskii S. V.
Slysh Viacheslav I.
Val'tts Irina E.
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