XZ Cygni 1965-2002

Physics

Scientific paper

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Rr Lyrae Stars: Light Curves, Period Variations

Scientific paper

The RR Lyrae-type star XZ Cygni has long been of interest to AAVSO observers because of its well-known tendency for dramatic period variations and the changes in the shape of its light curve due to a pronounced Blazhko effect. The AAVSO has monitored XZ Cyg closely for 38 years amassing a large volume of data on this star in the AAVSO International Database. These data result in 613 maxima timings which are analyzed in this document.

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