Search for Evolutionary Changes in the Periods of Cepheids: BY Cas
- 作者: Berdnikov L.N.1
-
隶属关系:
- Sternberg Astronomical Institute
- 期: 卷 45, 编号 9 (2019)
- 页面: 593-601
- 栏目: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191516
- DOI: https://doi.org/10.1134/S1063773719090019
- ID: 191516
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详细
For the low-amplitude Cepheid BY Cas we have constructed an O − C diagram spanning a time interval 123 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 increase in the period, dP/dt = +0.985 (±0.091) s yr−1, which points to the third crossing of the instability strip. The pulsation stability test proposed by Lombard and Koen (1993) confirms that the period increase is real.
作者简介
L. Berdnikov
Sternberg Astronomical Institute
编辑信件的主要联系方式.
Email: berdnik@sai.msu.ru
俄罗斯联邦, Universitetskii pr. 13, Moscow, 119992
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