Hostname: page-component-84b7d79bbc-g78kv Total loading time: 0 Render date: 2024-07-27T16:16:35.326Z Has data issue: false hasContentIssue false
  • English
  • Français

Galactic Background Radiation at 2 cm and Thermal Electrons in the Galaxy

Published online by Cambridge University Press:  14 August 2015

H. Hirabayashi
H. Hirabayashi*
Affiliation:
Tokyo Astronomical Observatory, Tokyo, Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The galactic background radiation at 4.2 and 15.5 GHz was observed with a resolution of 11′ at nine points on the galactic equator free of confusion from discrete sources. Relative amounts of thermal and nonthermal radiation were determined, and conditions in the interstellar gas are discussed.

Type
Part 1: The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 187 - 189
Copyright
Copyright © Reidel 1974 

References

Gordon, M. A. and Gottesman, S. T.: 1971, Astrophys. J. 168, 361.Google Scholar
Hirabayashi, H., Yokoi, H., and Morimoto, M.: 1972, Nature Phys. Sci. 237, 54.CrossRefGoogle Scholar
Jackson, P. D. and Kerr, F. J.: 1971, Astrophys. J. 168, 29.Google Scholar