Abstract
The galactic continuum radiation between lII = 21° and lII = 31° has been surveyed at 4,170 MHz with a beam width of 11 min of arc using the 30 m parabolic antenna of the Kashima Station of the Radio Research Laboratories. The survey will be extended to cover a much wider region, but some interesting results have already been obtained, and are presented here.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on SpringerLink
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Westerhout, G., Bull. Astron. Inst. Neth., 14, 215 (1958).
Hill, E. R., Slee, O. B., and Mills, B. Y., Austral. J. Phys., 11, 121 (1958).
Penzias, A. A., and Wilson, R. W., Astrophys. J., 146, 666 (1966).
Hill, E. R., Austral. J. Phys., 21, 735 (1968).
Beard, M., and Kerr, F. J., Austral. J. Phys., 22, 530 (1969).
Kesteven, M. J. L., Austral. J. Phys., 21, 739 (1968).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
HIRABAYASHI, H., OJIMA, T. & MORIMOTO, M. Galactic Background at 4 GHz. Nature 223, 49–51 (1969). https://doi.org/10.1038/223049a0
Received:
Revised:
Issue date:
DOI: https://doi.org/10.1038/223049a0
This article is cited by
-
Cosmic-ray electrons and galactic radio noise: Some problems
La Rivista del Nuovo Cimento (1975)
-
Measuring the spectral index of distributed cosmic radio emission at decimeter wavelengths
Radiophysics and Quantum Electronics (1975)
-
Galactic Background at 15 GHz
Nature Physical Science (1972)