The Analysis of Three Novae: Old Novae Q Cyg, DI Lac and N Cyg 1992 = V1974 Cyg

  • V. P. Goransky
  • S. Yu. Shugarov
  • E. S. Dmitrienko
  • E. P. Pavlenko
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 218)


The analysis of periodicity of three novae stars is carried out using the photometric observations. The archive plates of the Moscow Sternberg Institute collection, BVR-observations carried out at TV-complex of 0.5-m Maksutov telescope of Crimean observatory (Abramenko et al, 1988), and UBV RI- and W BV R- electrophotometric observations carried out at 0.6m, and 1.25-m reflectors of Crimea and 0.48-m, and 1.0-m reflectors of Tien-Shan observatory were used for analysis.


Orbital Period Light Curve Crimean Astrophysical Observatory Photometric Observation Orbital Periodicity 
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Copyright information

© Springer Science+Business Media Dordrecht 1997

Authors and Affiliations

  • V. P. Goransky
    • 1
  • S. Yu. Shugarov
    • 1
  • E. S. Dmitrienko
    • 2
  • E. P. Pavlenko
    • 2
  1. 1.Sternberg State Astronomical InstituteMoscow V-234Russia
  2. 2.Crimean Astrophysical ObservatoryNaychnii, CrimeaUkraine

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