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The Spectrum of CH Cygni – A Search for Rapid Line Variations

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The Symbiotic Phenomenon

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 145))

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Abstract

The spectacular changes of CH Cyg spectrum during the last period of activity and the flickering in short wavelength light suggest the possibility of rapid line variations (Walker et al.,1969). In November 1982 a series of spectral observations has been accomplished at Rozhen Observatory to investigate the subject.

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References

  • Chochol,D.,Hric,L.,Skopal,A. and Papousek,J.,1984,Contr. Astron. Obs, Scalnate Pleso,12,261

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  • Walker,G.,A.,H.,Morris,S.,C. and Younger,P.,E.,1969,Ap. J.,156, No.1,Part1

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© 1988 Kluwer Academic Publishers

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Tomov, T., Raikova, D. (1988). The Spectrum of CH Cygni – A Search for Rapid Line Variations. 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_42

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  • DOI: https://doi.org/10.1007/978-94-009-2969-2_42

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7833-7

  • Online ISBN: 978-94-009-2969-2

  • eBook Packages: Springer Book Archive

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