Dear colleagues! I would like to send you observations of a new variable star (Brh V83), 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 V83 165612.1 +035307 (J2000) 11.0 12.0 (CCD) SR comments: Brh V83: GSC 393 2695 The comparison star is GSC 393 2444 (11.8 mag), which has been checked for constant brightness. The red colour (USNO A2.0 r: 9.6, b: 12.5) and the apparently slow change of brightness suggest a SR-variable. object YYMMDD(UT) mag (CCD) code Brh V83 000702.8913 11.80 Brh.BAV Brh V83 000706.8926 11.81 Brh.BAV Brh V83 000717.8690 11.71 Brh.BAV Brh V83 000722.8774 11.62 Brh.BAV Brh V83 000731.8663 11.32 Brh.BAV Brh V83 000809.8760 11.20 Brh.BAV Brh V83 000814.8426 11.07 Brh.BAV Brh V83 000816.8357 11.07 Brh.BAV Brh V83 000819.8329 10.94 Brh.BAV Brh V83 000820.8357 10.98 Brh.BAV Brh V83 010614.9413 12.01 Brh.BAV Brh V83 010620.9378 11.89 Brh.BAV Brh V83 010621.9260 11.87 Brh.BAV Brh V83 010623.9350 11.81 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html