Add to ORKGUsing the Very Large Array1 and the Australia Telescope we have searched for the H92 α recombination line from 14 external galaxies and detected the line in 9 of them. All the detected galaxies have starburst nuclei and the line emission is only from the nuclear region. No line was detected in two well known Seyfert II galaxies that were searched to similar sensitivity levels
Radio recombination lines are known to be observable at positions along the galactic ridge which are...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
Using the Very Large Array with an angular resolution of 3", we have detected the hydrogen recombina...
Restricted Access. The central regions of the Galaxy and galaxies, Proceedings of the 184th symposiu...
Using the Very Large Array with an angular resolution of ~3", we have detected the hydrogen recombin...
We have detected the radio recombination lines H91α and H92α with rest frequencies of 8.6 GHz and 8....
Sorry, the full text of this article is not available here. Please click on the alternative location...
Using the Very Large Array (VLA) with an angular resolution of 3", we have detected the hydrogen rec...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
We have detected the radio recombination lines H91-alpha and H92-alpha with rest frequencies of 8.6 ...
Open Access.Context: Gas ionized by starburst activity radiates radio recombination lines (RRLs), fr...
Open AccessContext. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio ...
MSc (Space Physics), North-West University, Potchefstroom CampusThe role that high-mass stars play i...
Context. Gas ionized by starburst activity radiates radio recombination lines (RRLs), from which on...
Radio recombination lines are known to be observable at positions along the galactic ridge which are...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
Using the Very Large Array with an angular resolution of 3", we have detected the hydrogen recombina...
Restricted Access. The central regions of the Galaxy and galaxies, Proceedings of the 184th symposiu...
Using the Very Large Array with an angular resolution of ~3", we have detected the hydrogen recombin...
We have detected the radio recombination lines H91α and H92α with rest frequencies of 8.6 GHz and 8....
Sorry, the full text of this article is not available here. Please click on the alternative location...
Using the Very Large Array (VLA) with an angular resolution of 3", we have detected the hydrogen rec...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
We have detected the radio recombination lines H91-alpha and H92-alpha with rest frequencies of 8.6 ...
Open Access.Context: Gas ionized by starburst activity radiates radio recombination lines (RRLs), fr...
Open AccessContext. Hydrogen ionized by young, high-mass stars in starburst galaxies radiates radio ...
MSc (Space Physics), North-West University, Potchefstroom CampusThe role that high-mass stars play i...
Context. Gas ionized by starburst activity radiates radio recombination lines (RRLs), from which on...
Radio recombination lines are known to be observable at positions along the galactic ridge which are...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...