
TY  - JOUR
A1  - Rishbeth, H 
T1  - Radio Emission from the Vela?Puppis Region
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1958
VL  - 11
IS  - 4
SP  - 550
EP  - 563
KW  - 
UR  - https://doi.org/10.1071/PH580550 
N2  - The Vela-Puppis region has been surveyed with Mills Cross radio telescopes, and radio isophotes plotted at two wavelengths. Many discrete sources have been observed. Several H II regions have been detected in emission at 3·5 m and in absorption at 15·2 m; the radiation from such objects is of thermal origin. The outstanding feature of this region is a group of strong non-thermal sources near the galactic equator. These are superimposed on an intense belt of radiation along the equator, and this, too, is certainly non-thermal in origin. Some correlation with galactic structure is suggested. 
ER  -

