Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-12T19:54:39.992Z Has data issue: false hasContentIssue false
  • English
  • Français

The Galactic Plane Radio Source G321.48 + 1.02: is it Extragalactic?

Published online by Cambridge University Press:  25 April 2016

J. L. Caswell  and
R. T. Stewart
J. L. Caswell
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121
R. T. Stewart
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121
Get access Rights & Permissions [Opens in a new window]

Abstract

strong non-thermal radio sources at low galactic latitude may be young galactic supernova remnants or else distant extragalactic objects located in the direction of the galactic plane merely by chance. Here, we have imaged G321.48 + 1.02 with the Australia Telescope in order to distinguish between these alternatives for this source.

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 10 , Issue 1 , 1992 , pp. 21 - 23
Copyright
Copyright © Astronomical Society of Australia 1992

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Caswell, J.L., and Haynes, R.F., 1987, Astron. Astrophys., 171, 261.Google Scholar
Caswell, J.L., Haynes, R.F. and Clark, D.H., 1975, Aust. J. Phys., 28, 633.Google Scholar
Caswell, J.L., and Stewart, R.T., 1991, Proc Astron. Soc. Aust., 9, 103.Google Scholar
Clark, D.H. and Crawford, D.F., 1974, Aust. J. Phys., 27, 713.Google Scholar
Haynes, R.F., Caswell, J.L. and Simons, L.W.J., 1979, Aust J. Phys., Astrophys. suppl. number 48, 1.Google Scholar