Three-colour photometry of the eclipsing binary system RZ Cassiopeiae.

Physics

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Scientific paper

Three-colour differential photometry was performed of the short-period eclipsing binary system RZ Cas and UBV light curves are secured. The O-C values of recent primary minima indicate that the period of RZ Cas has been constant for the period including the authors' observations and is somewhat shorter than that listed in GCVS. A new ephemeris for the primary minimum has been determined. A discussion of the totality of the primary minimum is also given.

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