Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientific paper
2011-02-24
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
22 pages, 13 figures. Accepted for publication in Astrophysics and Space Science
Scientific paper
10.1007/s10509-011-0662-5
Sensitive spectral observations made in two frequency bands near 6.0 and 17.6 GHz are described for Orion and W51. Using frequency switching we were able to achieve a dynamic range in excess of 10,000 without fitting sinusoidal or polynomial baselines. This enabled us to detect lines as weak as T$_{A} ~1mK in these strong continuum sources. Hydrogen recombination lines with $\Delta n$ as high as 25 have been detected in Orion. In the Orion data, where the lines are stronger, we have also detected a systematic shift in the line center frequencies proportional to linewidth that cannot be explained by normal optical depth effects.
Avery Lorne W.
Bell Moley B.
MacLeod John M.
Vallee Jacques P.
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