Search for Evolutionary Changes in the Periods of Cepheids: CF Cas
- Authors: Berdnikov L.N.1, Pastukhova E.N.2
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Affiliations:
- Sternberg Astronomical Institute
- Institute of Astronomy
- Issue: Vol 45, No 2 (2019)
- Pages: 92-103
- Section: Article
- URL: https://journal-vniispk.ru/1063-7737/article/view/191078
- DOI: https://doi.org/10.1134/S1063773719020014
- ID: 191078
Cite item
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.
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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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