Dear colleagues! I would like to send you observations of a new variable star (Brh V93), 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 V93 182203.3 +072137 (J2000) 12.7-13.0 (CCD) SR comments: Brh V93: GSC 444 2502 The comparison star is GSC 444 2300 (12.3 mag), which has been checked for constant brightness. The colour (USNO A2.0 r: 11.8, b: 14.2) and the apparently slow change of brightness suggest a SR-variable. Other types of variability cannot be excluded. object YYMMDD(UT) mag (CCD) code Brh V93 010625.0014 12.86 Brh.BAV Brh V93 010625.9674 12.80 Brh.BAV Brh V93 010626.9660 12.93 Brh.BAV Brh V93 010705.9576 12.95 Brh.BAV Brh V93 010709.9611 12.80 Brh.BAV Brh V93 010714.9688 12.74 Brh.BAV Brh V93 010715.9417 12.67 Brh.BAV Brh V93 010717.9556 12.68 Brh.BAV Brh V93 010721.9472 12.65 Brh.BAV Brh V93 010728.9444 12.73 Brh.BAV Brh V93 010730.9521 12.81 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html