
%0 Journal Article
%A Caswell, JL 
%A Haynes, RF 
%T Survey of OH Masers at 1665 MHz. II. Galactic Longitude 340o to the Galactic Centre
%J Australian Journal of Physics
%D 1983/06/01
%V 36
%N 3
%P 361-400
%K 
%R https://doi.org/10.1071/PH830361B
%U https://www.publish.csiro.au/paper/PH830361B 
%X The galactic plane from longitude 340° through the galactic centre to longitude + 2° has been searched for OH on the 1665 MHz transition. Forty-nine OH maser emission sources were detected and these have now been studied on all four OH ground-state transitions. Most of the masers are associated with regions of star formation (type I) while three may be examples of late-type stars (type II OH/IR) with unusually strong main-line emission 
