Recent activity on CH Cygni

Astronomy and Astrophysics – Astronomy

Scientific paper

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H Alpha Line, Stellar Oscillations, Stellar Spectra, Ubv Spectra, Variable Stars, Balmer Series, Continuous Spectra, Cygnus Constellation, M Stars

Scientific paper

UBV and Hα photometry from the summer of 1982 indicate that activity has increased on CH Cygni. A B-V colour of +0.30±0.05 was measured; the amplitude of short time-scale "flickering" has grown since the 1977 outburst, more so in the B and V bandpasses than in the U. These recent developments are interpreted as ramifications of the binary nature of CH Cyg.

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