2008BAVSR..57..150M

On CCD images of GM And, which were taken at the observatory Calar Alto with Stroemgren- filters, the suspected variable NSV 26190 was observed too. NSV 26190 was discovered by Schmidt et al. (1990). Taking further observations during 3 nights at the observatory Hoher List, NSV 26190 was found to be a short period eclipsing binary of type EW. Its period was determined to 0.353401113 d ±0.000973 d, first epoch 2454337.3854 [JD], its magnitude (y filter) is 15.15 mag (maximum), 15 .60 mag (minimum 1), and 15.52 (minimum 2).