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Stepanian’s Star

  • Peter Rovithis
Conference paper
Part of the NATO Advanced Study Institutes Series book series (ASIC, volume 69)

Abstract

The light curve of the new variable star that Stepanian discovered in 1979 is given based on photoelectric observations made at Kryonerion Astronomical Station of the National Observatory of Athens during April 1980. The variable is an eclipsing binary of short period and the differences between primary minimum and a mean value at maximum were found to be 2 . m 425 in B and 2 . m 925 in V.

Keywords

Light Curve Variable Star Cataclysmic Variable National Observatory Image Tube 
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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References

  1. Contopoulos, G. and Banos, C.: 1976, Sky and Telescope, 51, p. 154.ADSGoogle Scholar
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  8. Wenzel, W. W.: 1979, I.B.V.S. No. 1720.Google Scholar

Copyright information

© D. Reidel Publishing Company 1981

Authors and Affiliations

  • Peter Rovithis
    • 1
  1. 1.National Observatory of AthensAthensGreece

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