Averaged light curves drawn from visual observations by T. Kato, 341 estimates distributed between 1985 August and 1993 Novevmer. The observations were done using a 10-cm and 20-cm reflectors.
The best determined period of 66.81 d was used in folding the light curve. Alternating waves are evident which are characterstic to RV Tau-type variable stars.
Variable stars in M5
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