Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-26T03:28:29.406Z Has data issue: false hasContentIssue false
  • English
  • Français

Variable Radio Emission from X-Ray Sources

Published online by Cambridge University Press:  12 April 2016

L. L. E. Braes  and
G. K. Miley
L. L. E. Braes
Affiliation:
Leiden
G. K. Miley
Affiliation:
Leiden

Extract

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.

Dr. KELLOGG has just described some exciting new observations of X-ray sources made with the UHURU satellite. We shall now move some nine orders of magnitude in wavelength to the opposite end of the electromagnetic spectrum and report measurements of weak radio emission from some of the objects he mentioned. For the detection of weak sources most radio telescopes are not noise limited, but are confusion limited by their low resolution. The aperture synthesis technique minimizes this problem because it enables one to pinpoint the position of weak sources to the order of one second of arc.

Type
III. Rapid and Ultrarapid Variables (Including X-Rax Sources)
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 173 - 175
Copyright
Copyright © Cambridge University Press 1971

References

Bidelman, W. P., and Weitenbeck, A. J., 1971, IAU Circ. No. 2345.Google Scholar
Braes, L. L. E., and Brouw, W. N., 1971, Astron. Astrophys. 12, 320.Google Scholar
Braes, L. L. E., and Miley, G. K., 1971a, Nature, 232, 246.CrossRefGoogle Scholar
Braes, L. L. E., and Miley, G. K., 1971b, Astron. Astrophys. 14, 160.Google Scholar
Dolan, J. F., 1970, Space Sci. Rev., 10, 830.Google Scholar
Hjellming, R. M., and Wade, C. M., 1971a, Astrophys. J. 164, L1.CrossRefGoogle Scholar
Hjellming, R. M., and Wade, C. M., 1971b, Astrophys. J. 168, L21.CrossRefGoogle Scholar
Hjellming, R. M., and Wade, C. M., 1971c, submitted to Astrophys. J. Google Scholar