Volume 47 number 1 (2019)
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A study of the suspected variable star Ross 114 (NSV 13523) has been carried out. The star is confirmed to be a variable with an amplitude of about 2.5 magnitudes in B. Photometry and light curves from CCD images and archival photographic plates are presented. The observations show the star is a long period variable with a period of about 296 days.