Search for Evolutionary Changes in the Periods of Cepheids: CF Cas


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Abstract

For the classical Cepheid CF Cas we have constructed an O-C diagram spanning a time interval of 129 years. The O-C diagram has the shape of a parabola, which has made it possible to determine for the first time the quadratic light elements and to calculate the rate of evolutionary decrease in the period, dP/dt = −0.050 (±0.006) syr−1, in agreement with the results of theoretical calculations for the second crossing of the instability strip. The available data reduced by the Eddington-Plakidis method show no random period fluctuations, i.e., the parabola on the O-C diagram reflects a real evolutionary decrease in the period.

About the authors

L. N. Berdnikov

Sternberg Astronomical Institute

Author for correspondence.
Email: berdnik@sai.msu.ru
Russian Federation, Universitetskii pr. 13, Moscow, 119992

E. N. Pastukhova

Institute of Astronomy

Email: berdnik@sai.msu.ru
Russian Federation, Pyatnitskaya ul. 48, Moscow, 119017

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