Dear colleagues! I would like to send you observations of a new variable star (Brh V77), 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 V77 192442.7 +040655.2 (J2000) 12.1 12.7 (CCD) SR comments: Brh V77: GSC 473 5480 The comparison star is GSC 473 5556 (12.2 mag), which has been checked for constant brightness. The red colour (USNO A2.0 r: 11.1, b: 15.1) and the apparently slow change of brightness suggest a SR-variable. object YYMMDD(UT) mag (CCD) code Brh V77 000706.9954 12.36 Brh.BAV Brh V77 000717.9718 12.14 Brh.BAV Brh V77 000722.9801 12.16 Brh.BAV Brh V77 000731.9690 12.11 Brh.BAV Brh V77 000801.9642 12.18 Brh.BAV Brh V77 000809.9788 12.22 Brh.BAV Brh V77 000811.9433 12.21 Brh.BAV Brh V77 000819.9357 12.20 Brh.BAV Brh V77 000820.9385 12.21 Brh.BAV Brh V77 010621.0406 12.73 Brh.BAV Brh V77 010624.0378 12.64 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html