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


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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.

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L. Berdnikov

Sternberg Astronomical Institute

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Email: berdnik@sai.msu.ru
俄罗斯联邦, Universitetskii pr. 13, Moscow, 119992

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