Dear colleagues! I would like to send you observations of a new variable star (Brh V74), 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 V74 165612.1 +035307 (J2000) 10.3 11.4 (CCD) SR comments: Brh V74: GSC 393 2695 The comparison star is GSC 393 2641 (12.1 mag), which has been checked for constant brightness. The red colour (USNO A 2.0: r:9.6, b:12.5) and the apparently slow variation in brightness suggest a SR-variable. object YYMMDD(UT) mag (CCD) code Brh V74 000702.8913 11.21 Brh.BAV Brh V74 000706.8926 11.14 Brh.BAV Brh V74 000717.8690 11.19 Brh.BAV Brh V74 000722.8774 10.99 Brh.BAV Brh V74 000731.8663 10.73 Brh.BAV Brh V74 000801.8614 10.72 Brh.BAV Brh V74 000809.8760 10.56 Brh.BAV Brh V74 000814.8426 10.41 Brh.BAV Brh V74 000816.8357 10.40 Brh.BAV Brh V74 000819.8329 10.37 Brh.BAV Brh V74 000820.8357 10.33 Brh.BAV Brh V74 010614.9413 11.38 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html