Hostname: page-component-848d4c4894-sjtt6 Total loading time: 0 Render date: 2024-07-03T13:19:05.906Z Has data issue: false hasContentIssue false
  • English
  • Français

G357.7-0.1—a Double-lobed Radio Source?

Published online by Cambridge University Press:  25 April 2016

J. L. Caswell ,
M. J. Kesteven ,
T. R. Bedding  and
A. J. Turtle
J. L. Caswell
Affiliation:
Division of Radiophysics, CSIRO, Sydney
M. J. Kesteven
Affiliation:
Division of Radiophysics, CSIRO, Sydney
T. R. Bedding
Affiliation:
School of Physics, University of Sydney
A. J. Turtle
Affiliation:
School of Physics, University of Sydney
Get access Rights & Permissions [Opens in a new window]

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.

Type
Miscellaneous Radio Astronomy
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 2 , 1989 , pp. 184 - 186
Copyright
Copyright © Astronomical Society of Australia 1989

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

Becker, R. H. and Helfand, D. J., 1985, Nature, 313, 115.CrossRefGoogle Scholar
Bridle, A. H., Fomalont, E. B. and Cornwell, T. J., 1981, Astron. J., 86, 1294.CrossRefGoogle Scholar
Caswell, J. L., Clark, D. H. and Crawford, D. F., 1975, Aust. J. Phys., Astrophys. suppl., No. 37, 39.Google Scholar
Caswell, J. L., Haynes, R. F., Milne, D. K. and Wellington, K. J., 1980, Mon. Not. R. Astron. Soc., 190, 881.Google Scholar
Clark, D. H. and Caswell, J. L., 1976, Mon. Not. R. Astron. Soc., 174, 267.Google Scholar
Fanaroff, B. L. and Riley, J. M., 1974, Mon. Not. R. Astron. Soc., 167, 31P.CrossRefGoogle Scholar
Fedorenko, V. N. and Zentsova, A. S., 1986, Sov. Astron., 30, 24.Google Scholar
Green, D. A. and Gull, S. F., 1984, Nature, 312, 527.Google Scholar
Green, D. A. and Gull, S. F., 1986, Nature, 320, 42.CrossRefGoogle Scholar
Helfand, D. J. and Becker, R. H., 1985, Nature, 313, 118.Google Scholar
Mills, B. Y., 1981, Proc. Astron. Soc. Aust., 4, 156.Google Scholar
Milne, D. K., 1970, Aust. J. Phys., 23, 425.Google Scholar
Milne, D. K., Goss, W. M., Haynes, R. F., Wellington, K. J., Caswell, J. L. and Skellern, D. J., 1979, Mon. Not. R. Astron. Soc., 188, 437.Google Scholar
Shaver, P. A., Salter, C. J., Patnaik, A. R., van Gorkom, J. H. and Hunt, G. C, 1985a, Nature, 313, 113.Google Scholar
Shaver, P. A., Pottasch, S. R., Salter, C. J. Patnaik, A. R., van Gorkom, J. H. and Hunt, G. C., 1985b, Astron. Astrophys. 147, L23.Google Scholar
van Breugel, W. J. M. and Fomalont, E.B., 1984, Astrophys. J. (Letts), 282, L55.CrossRefGoogle Scholar
Weiler, K. W. and Panagia, N., 1980, Astron. Astrophys., 90, 269.Google Scholar