Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...8925086s&link_type=abstract
Unknown
Astronomy and Astrophysics
Astronomy
Emission Spectra, Infrared Astronomy, Line Spectra, Microwave Spectra, Molecular Spectra, Orion Nebula, Rotational Spectra, Electron Transitions, Methyl Alcohol, Sulfur Dioxides
Scientific paper
Emission lines from the Orion core are analyzed. Peak main beam brightness temperatures are 7 and 9 K in a 25 sec beam. The widths and center velocities of these lines are similar to those of recently detected transitions. The SO2 emission is best modelled by an optically thick, beam diluted source. The third line, not yet identified, has its peak main beam brightness temperature at 3.5 K.
Genzel Reinhard
Graf Urs U.
Harris Andrew I.
Jaffe Daniel T.
Stutzki Juergen
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