We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (30 THz) that are useful to radio astronomers working at high frequencies. In particular, the fine structure of hydrogen has been treated explicitly for the First time in this radio-astronomical context
Open AccessContext. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio ...
Restricted Access. The central regions of the Galaxy and galaxies, Proceedings of the 184th symposiu...
This dissertation resolves a mystery in cosmic radio recombination line observations reported by Bel...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
Observations of recombination lines form normal H II regions, extended H II regions, nonthermal sour...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
International audienceWe report the detection of stimulated hydrogen radio recombination line (RRL) ...
We report the detection of stimulated hydrogen radio recombination line (RRL) emission from ionized ...
Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful r...
MSc (Space Physics), North-West University, Potchefstroom CampusThe role that high-mass stars play i...
In a previous paper we presented a low-resolution (2°×2°) survey of radio recombination lines (RRLs)...
The discovery of the first naturally occurring high gain hydrogen recombination line (HRL) maser, in...
We explore the possibility of detecting hydrogen radio recombination lines from 0 < z < 10 qua...
A survey of ten galactic HII regions provided the most extensive high frequency (near 8.6 GHz) recom...
Open AccessContext. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio ...
Restricted Access. The central regions of the Galaxy and galaxies, Proceedings of the 184th symposiu...
This dissertation resolves a mystery in cosmic radio recombination line observations reported by Bel...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
Observations of recombination lines form normal H II regions, extended H II regions, nonthermal sour...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
International audienceWe report the detection of stimulated hydrogen radio recombination line (RRL) ...
We report the detection of stimulated hydrogen radio recombination line (RRL) emission from ionized ...
Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful r...
MSc (Space Physics), North-West University, Potchefstroom CampusThe role that high-mass stars play i...
In a previous paper we presented a low-resolution (2°×2°) survey of radio recombination lines (RRLs)...
The discovery of the first naturally occurring high gain hydrogen recombination line (HRL) maser, in...
We explore the possibility of detecting hydrogen radio recombination lines from 0 < z < 10 qua...
A survey of ten galactic HII regions provided the most extensive high frequency (near 8.6 GHz) recom...
Open AccessContext. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio ...
Restricted Access. The central regions of the Galaxy and galaxies, Proceedings of the 184th symposiu...
This dissertation resolves a mystery in cosmic radio recombination line observations reported by Bel...