Part of the Lecture Notes in Physics book series (LNP, volume 125)
16 Lacertae: An eclipsing system with a β Cephei primary
A model is presented of the 16 Lacertae system which is shown to be an eclipsing variable with a g Cephei primary.
KeywordsOrbital 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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© Springer-Verlag 1980