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- W2370009866 abstract "The light variations of the W UMa system V523 Cas were monitored.In our observations the system showed appreciable periodic light variability.By using the methods of the Phase Dispersion Minimization (PDM) and Fourier analysis(PERIOD04),the rotational periods of these stars were determined.The color curve indicates that the system becomes redder by 0m.07 and 0m.06 during primary and secondary eclipse,respectively.This indicates that regions of cooler gas are visible at such times.The maximum following the secondary minimum is 0m.022 brighter in B and 0m.018 bright in V." @default.
- W2370009866 created "2016-06-24" @default.
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- W2370009866 date "2009-01-01" @default.
- W2370009866 modified "2023-09-28" @default.
- W2370009866 title "Study on Photometry of the W UMa System V523 Cas" @default.
- W2370009866 hasPublicationYear "2009" @default.
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