Dear colleagues! I would like to send you observations of a new variable star (Brh V84), 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 V84 190053.0 +071203 (J2000) 12.3-12.7 (CCD) SR comments: Brh V84: GSC 474 323 The comparison star is GSC 474 195 (11.9 mag), which has been checked for constant brightness. The red colour (USNO A2.0 r: 11.4, b: 14.0) 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 V84 010625.0281 12.67 Brh.BAV Brh V84 010625.9940 12.54 Brh.BAV Brh V84 010626.9926 12.67 Brh.BAV Brh V84 010703.9753 12.38 Brh.BAV Brh V84 010705.9843 12.32 Brh.BAV Brh V84 010709.9878 12.68 Brh.BAV Brh V84 010714.9954 12.63 Brh.BAV Brh V84 010715.9683 12.57 Brh.BAV Brh V84 010717.9822 12.43 Brh.BAV Brh V84 010721.9739 12.34 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html