Dear colleagues, time series photometry of the field of V672 Her was searched for new variable stars as outlined in earlier emails (cf. for example vsnet-newvar 1857). 1 new variable star was found. Pej 021 = GSC 1037:0744 RA = 18:44:58.0, Dec = +13:40:32 (J2000), USNO B1.0 gives B-R = 4.1 mag. The star is in IRAS PSC catalogue. 2MASS gives J-K = 1.43 mag. The colours and lack of short term variability suggest semiregular nature. The following observations are differentials against GSC 1037:530. The data were averaged on nightly basis (50-200 images per night), thus the internal error is small. 20020729.94 -1.17Ic (Petr Sobotka) 20020731.93 -1.20Ic (Petr Sobotka) 20030626.94 -1.10Ic (Ondrej Pejcha) 20030706.88 -1.02Ic (Ondrej Pejcha) 20030713.95 -1.00Ic (Ondrej Pejcha) 20030715.01 -0.99Ic (Ondrej Pejcha) 20030720.94 -1.02Ic (Ondrej Pejcha) 20020729.95 -0.31Rc (Petr Sobotka) 20030626.94 -0.23Rc (Ondrej Pejcha) 20030706.88 -0.11Rc (Ondrej Pejcha) 20030713.95 -0.08Rc (Ondrej Pejcha) 20030715.01 -0.08Rc (Ondrej Pejcha) 20030720.94 -0.11Rc (Ondrej Pejcha) 20020729.94 0.59V (Petr Sobotka) 20030626.94 0.67V (Ondrej Pejcha) 20030706.88 0.83V (Ondrej Pejcha) 20030713.94 0.93V (Ondrej Pejcha) 20030715.01 0.88V (Ondrej Pejcha) 20030720.92 0.84V (Ondrej Pejcha) Best regards, Ondrej Pejcha
vsnet-adm@kusastro.kyoto-u.ac.jp