Radial Velocities of CH Cygni Just as the Jets Appeared
The period of maximum brightness of CH Cygni which started in mid 1981 finished at the end of July 1984, when sudden drop by about 1 mag was observed (Fig.1). At the same time a radio outburst has occured and the jet structure has developed (Taylor et al.1986). The Toruń Observatory has recorded the...
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Veröffentlicht in: | International Astronomical Union Colloquium 1988, Vol.103, p.225-226 |
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Sprache: | eng |
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