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Continued Radio Activity from CH Cygni

  • A. R. Taylor
  • E. R. Seaquist
  • S. J. Kenyon
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)

Abstract

Following the discovery of the radio outburst and jet formation from CH Cygni in 1984, continued radio monitoring has been carried out with the Very Large Array. We present the preliminary results of these observations, including a high resolution image of the jet in 1986 -1.5 years after the initial outburst. The star has remained active in the radio, undergoing at least one additional outburst. The radio jet has continued to expand and shows evidence of multiple episodes of ejection along the same axis.

Keywords

High Resolution Image Large Array Multiple Episode Radio Image Radio Flux 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

References

  1. Selvelli, P.L. and Hack, M. 1985 Astronomy Express ,1.Google Scholar
  2. Taylor, A.R., Seaquist, E.R. and Mattei, J.A. 1986, Nature ,319, 38.ADSCrossRefGoogle Scholar
  3. Tomov, T. 1984 Inf. Bull, of Var. Stars ,No. 2610.Google Scholar

Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • A. R. Taylor
    • 1
  • E. R. Seaquist
    • 2
  • S. J. Kenyon
    • 3
  1. 1.Department of PhysicsUniversity of CalgaryCanada
  2. 2.Department of AstronomyUniversity of TorontoCanada
  3. 3.Harvard-Smithsonian Center for AstrophysicsUSA

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