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 TA 3c 1 mK in these strong continuum sources. Hydrogen recombination lines with 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.Peer reviewed: YesNRC publication: Ye
Over the past forty years, investigations of radio recombination lines have become an effective way ...
Observations of recombination lines form normal H II regions, extended H II regions, nonthermal sour...
We use the Low Frequency Array to perform a systematic high spectral resolution investigation of the...
Sensitive spectral observations made in two frequency bands near 6.0 and 17.6 GHz are described for ...
We critically analyze the Bell et al. findings on "anomalous" widths of high-order Hydrogen radio re...
Problems where impact broadened radio recombination lines appeared narrower than predicted first sho...
In 1967 Griem gave a general formula for the electron-impact broadening of radio recombination lines...
This dissertation resolves a mystery in cosmic radio recombination line observations reported by Bel...
On-the-fly mapping of cm-wave spectral lines has been implemented at the Tidbinbilla 70-m radio anten...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
We have conducted a line survey toward Orion KL using the Q-band receiver of the Tianma 65 m radio t...
The absorption line at 26 MHz observed by Konovalenko and Sodin towards Cas A was interpreted by Bla...
In a previous paper we presented a low-resolution (2°×2°) survey of radio recombination lines (RRLs)...
Sorry, the full text of this article is not available here. Please click on the alternative location...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
Observations of recombination lines form normal H II regions, extended H II regions, nonthermal sour...
We use the Low Frequency Array to perform a systematic high spectral resolution investigation of the...
Sensitive spectral observations made in two frequency bands near 6.0 and 17.6 GHz are described for ...
We critically analyze the Bell et al. findings on "anomalous" widths of high-order Hydrogen radio re...
Problems where impact broadened radio recombination lines appeared narrower than predicted first sho...
In 1967 Griem gave a general formula for the electron-impact broadening of radio recombination lines...
This dissertation resolves a mystery in cosmic radio recombination line observations reported by Bel...
On-the-fly mapping of cm-wave spectral lines has been implemented at the Tidbinbilla 70-m radio anten...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
We have conducted a line survey toward Orion KL using the Q-band receiver of the Tianma 65 m radio t...
The absorption line at 26 MHz observed by Konovalenko and Sodin towards Cas A was interpreted by Bla...
In a previous paper we presented a low-resolution (2°×2°) survey of radio recombination lines (RRLs)...
Sorry, the full text of this article is not available here. Please click on the alternative location...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
Observations of recombination lines form normal H II regions, extended H II regions, nonthermal sour...
We use the Low Frequency Array to perform a systematic high spectral resolution investigation of the...