
%0 Journal Article
%A McGee, RX 
%A M Newton, Lynette 
%A Brooks, JW 
%T Recombination Lines near 6 cm Wavelength in the Large Magellanic Cloud
%J Australian Journal of Physics
%D 1974/10/01
%V 27
%N 5
%P 729-736
%K 
%R https://doi.org/10.1071/PH740729
%U https://www.publish.csiro.au/paper/PH740729 
%X Recombination lines H 10901: have been detected in eight sources in the Large Cloud of Magellan. Low ratios of line temperature to continuum temperature, TL/Tc, were found in most of the sources and are attributed to the difficulty of obtaining a true continuum value when such a large area is encompassed by the telescope beam. In the 30Doradus nebula the ratio N(He+)/N(H+) was found to be no greater than O' 08, or less than half that previously recorded by radio observations. 
