Continued Radio Activity from CH Cygni
Part of the
Astrophysics and Space Science Library
book series (ASSL, volume 145)
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.
KeywordsHigh 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.
Selvelli, P.L. and Hack, M. 1985 Astronomy Express
Taylor, A.R., Seaquist, E.R. and Mattei, J.A. 1986, Nature
, 38.ADSCrossRefGoogle Scholar
Tomov, T. 1984 Inf. Bull, of Var. Stars
,No. 2610.Google Scholar
© Kluwer Academic Publishers 1988