Dear colleagues! I would like to send you observations of a new variable star (Brh V124), which I have discovered in a systematic CCD-based search for new variables. In each observing run typically 400 images are taken of several survey fields. The frames are processed automatically. Instruments: CCD-camera: Starlight Xpress SX (unfiltered) Telescope: Celestron-8 (20 cm Schmidt-Cassegrain) New variable star: new Brh V124 212544.1 +160211.1 (J2000) 12.2-14.2 (CCD) comments: Brh V124: GSC 1663 403 The comparison star is GSC 1663 145 (12.4 mag), which has been checked for constant brightness. The USNO-B1.0 magnitudes (b1mag: 14.56, b2mag: 16.89, r1mag: 11.42, r2mag: 10.95) and the following observations suggest a long period variable with a relatively high amplitude, maybe a Mira variable. object YYMMDD(UT) mag(CCD) code Brh V124 021008.8369 12.26 Brh.BAV Brh V124 021112.8161 13.42 Brh.BAV Brh V124 021113.8119 13.49 Brh.BAV Brh V124 021120.7563 13.56 Brh.BAV Brh V124 021123.7293 13.71 Brh.BAV Brh V124 021208.7216 14.22 Brh.BAV Brh V124 021208.7221 14.03 Brh.BAV Brh V124 021208.7226 14.21 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.lycos.de/klausbernhard/