Hostname: page-component-669899f699-tpknm Total loading time: 0 Render date: 2025-04-26T18:59:58.123Z Has data issue: false hasContentIssue false
  • English
  • Français

Apparent Relativistic Motion in Cygnus X-3

Published online by Cambridge University Press:  12 April 2016

R. E. Spencer
R. E. Spencer*
Affiliation:
University of Manchester, Jodrell Bank, Macclesfield, Cheshire SK 11 9DL, UK

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.

Weak and strong flaring has been observed at cm-wavelengths on Cygnus X-3. The weak flares seem to have different statistical properties to those of the strong flares. Previous observations have shown the ejection of radio emitting blobs at around 0.3c following major flares. However recent VLBA observations show apparent superluminal expansion and contraction during weak flaring.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 337 - 338
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Fender, R.P., Bell Burnell, S.J., & Waltman, E.B. 1997. Vistas in Ast. 41, 3–13.Google Scholar
Newell, S.J., Spencer, R.E., & Garrett, M.A. 1997. Vistas in Ast. 41, 57–63.Google Scholar
Ogley, R.N., Bell Burnell, S.J., & Newell, S.J. 1997. MNRAS, 285, 187–190.Google Scholar
Waltman, E., et al. 1996. AJ, 112, 2690–2698.Google Scholar