Search for Evolutionary Changes in the Periods of Cepheid: DX Gem
- Authors: Berdnikov L.N.1
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Affiliations:
- Sternberg Astronomical Institute
- Issue: Vol 45, No 7 (2019)
- Pages: 435-444
- Section: Article
- URL: https://journal-vniispk.ru/1063-7737/article/view/191391
- DOI: https://doi.org/10.1134/S1063773719070016
- ID: 191391
Cite item
Abstract
For the low-amplitude Cepheid DX Gem we have constructed an O - C diagram spanning a time interval of 120 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 = −0.808(±0.108) s yr−1, which points to the second crossing of the instability strip. The available data reduced by the Eddington-Plakidis method show random period fluctuations, ε/P ≈ 0.0072, whose amplitude on the O - C diagram is comparable to the amplitude of evolutionary changes.
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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
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