G357.7-0.1—a Double-lobed Radio Source?
- 1 January 1989
- journal article
- research article
- Published by Cambridge University Press (CUP) in Publications of the Astronomical Society of Australia
- Vol. 8 (2) , 184-186
- https://doi.org/10.1017/s1323358000023298
Abstract
The radio source G357.7-0.1 has commonly been regarded as a galactic supernova remnant; alternative interpretations have concentrated on the pronounced brightness gradient along its major axis. Analysis of our new map shows that this brightness gradient masks an even more crucial characteristic – symmetry about the centre – the key to a totally different interpretation.Keywords
This publication has 1 reference indexed in Scilit:
- Simultaneous Observations of Pulsar Intensity Variations at Parkes and OotacamundMonthly Notices of the Royal Astronomical Society, 1974