Abstract
A model is presented of the 16 Lacertae system which is shown to be an eclipsing variable with a g Cephei primary.
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References
Fitch, W.S. 1969, Ap. J., 158, 269.
Jerzykiewicz, M., Jarzebowski, T., Le Contel., J.-M. and Musielok, B. 1978, Comm. 27 I.A.U. Inf. Bull. Var. Stars, no. 1508.
Sterken, C. and Jerzykiewicz, M. 1979, these proceedings.
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© 1980 Springer-Verlag
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Jerzykiewicz, M. (1980). 16 Lacertae: An eclipsing system with a β Cephei primary. In: Hill, H.A., Dziembowski, W.A. (eds) Nonradial and Nonlinear Stellar Pulsation. Lecture Notes in Physics, vol 125. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-09994-8_11
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DOI: https://doi.org/10.1007/3-540-09994-8_11
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