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.
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References
Selvelli, P.L. and Hack, M. 1985 Astronomy Express ,1.
Taylor, A.R., Seaquist, E.R. and Mattei, J.A. 1986, Nature ,319, 38.
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© 1988 Kluwer Academic Publishers
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Taylor, A.R., Seaquist, E.R., Kenyon, S.J. (1988). Continued Radio Activity from CH Cygni. In: Mikolajewska, J., Friedjung, M., Kenyon, S.J., Viotti, R. (eds) The Symbiotic Phenomenon. Astrophysics and Space Science Library, vol 145. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2969-2_44
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DOI: https://doi.org/10.1007/978-94-009-2969-2_44
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7833-7
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