New maxima of CY Aquarii observed in August 1980 and accurate determination of a mean maximum.

Physics

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Intrinsic Variables, Pulsating Stars, Spectrum Variables, Pulsation Theory

Scientific paper

CY Aqr was observed in August 1980 by 11 members of the GEOS, who collected more than 7500 visual estimates leading to the determination of 237 maxima. A statistical processing enabled the influence of systematic errors to be considerably reduced: the standard deviations on timings of maxima are lower than 0.002 d for the best observers. This led to the determination of a particularly accurate mean maximum: JD hel. 2,444,465.4526(+/-3) d.

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