Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-30T03:48:13.331Z Has data issue: false hasContentIssue false
  • English
  • Français

High Resolution Observations of Low frequency Variables at 932 MHz

Published online by Cambridge University Press:  03 August 2017

Lars B. Bååth
Lars B. Bååth*
Affiliation:
Onsala Space Observatory, S-439 00 Onsala, Sweden

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.

Fifteen sources known to be varying at low frequencies have been observed at six epochs during 1983–84 with a global VLBI array. Some of the sources show structural variations similar to the superluminals. Beaming effect may therefore play an important role at low frequencies as well as at higher.

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 117 - 118
Copyright
Copyright © Reidel 1988 

References

Bååth, L.B. 1987, Superluminal Radio Sources, ed. Zensus, and Pearson, , Cambridge University Press, 206 Google Scholar
Ricket, B.J., Coles, W.A., and Bourgois, G. 1984, Astron. Astrophys., 134, 390 Google Scholar
Sholomitskii, G.B. 1965, Astron. Zh, 42, 673 Google Scholar