On the Question of the Behavior of O-C Residuals of Active Algol-like Binary RZ Cas

Physics – Space Physics

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Scientific paper

We present the analysis of the RZ Cassiopeia' O-C diagram for a 30 years period, which is based on the data published at AAVSO. The new parabolic light-elements are determined. Also, P-with-point was estimated. This enabled us to establish the value of M-with-point (the rate of the mass transfer between components of this eclipsing binary). Deviations from the parabola in the RZ Cas' O-C diagram have a wavelike trend. The pulsation of the primary component influences the scatter of O-C points, as well as it influences the eclipse' shape. Some physical points on such O-C behavior are presented.

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