Dear colleagues! I would like to send you observations of a new variable star (Brh V90), 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 V90 195359.4 +071444.9 (J2000) 12.0-12.4 (CCD) SR comments: Brh V90: GSC 493 629 The comparison star is GSC 493 799 (12.1 mag), which has been checked for constant brightness. The red colour (USNO A2.0 r: 11.4, b: 13.9) and the apparently slow change of brightness suggest a SR-variable. Other types of long period variability cannot be excluded. object YYMMDD(UT) mag (CCD) code Brh V90 010625.0647 12.17 Brh.BAV Brh V90 010626.0307 12.09 Brh.BAV Brh V90 010627.0293 12.21 Brh.BAV Brh V90 010628.0272 12.17 Brh.BAV Brh V90 010704.0119 12.37 Brh.BAV Brh V90 010705.0175 12.34 Brh.BAV Brh V90 010706.0210 12.35 Brh.BAV Brh V90 010710.0244 12.39 Brh.BAV Brh V90 010711.0147 12.37 Brh.BAV Brh V90 010715.0321 12.36 Brh.BAV Brh V90 010718.0189 12.29 Brh.BAV Brh V90 010722.0106 12.23 Brh.BAV Brh V90 010729.0078 12.04 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html