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16 Lacertae: An eclipsing system with a β Cephei primary

  • M. Jerzykiewicz
2. β Cephei and other Early-Type Variables
Part of the Lecture Notes in Physics book series (LNP, volume 125)

Abstract

A model is presented of the 16 Lacertae system which is shown to be an eclipsing variable with a g Cephei primary.

Keywords

Orbital Period Eclipse Phase Compute Depth Small Mass Ratio Radius Figure 
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. Fitch, W.S. 1969, Ap. J., 158, 269.Google Scholar
  2. Jerzykiewicz, M., Jarzebowski, T., Le Contel., J.-M. and Musielok, B. 1978, Comm. 27 I.A.U. Inf. Bull. Var. Stars, no. 1508.Google Scholar
  3. Sterken, C. and Jerzykiewicz, M. 1979, these proceedings.Google Scholar

Copyright information

© Springer-Verlag 1980

Authors and Affiliations

  • M. Jerzykiewicz
    • 1
  1. 1.Wroclaw University ObservatoryPoland

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