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Astrophysics

, Volume 16, Issue 3, pp 262–270 | Cite as

An unusual variable star: CH Cyg

  • L. S. Luud
Article

Conclusions

The existing observational data on CH Cyg agrees well with a model consisting of a semiregular M6 III giant and a white dwarf with a transient accretion disk formed at the time of the large maxima. The model can be tested by means of x-ray and speckle-interferometric observations.

Keywords

Observational Data Accretion Disk White Dwarf Variable Star Large Maximum 
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.

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Copyright information

© Plenum Publishing Corporation 1981

Authors and Affiliations

  • L. S. Luud

There are no affiliations available

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