Dear colleagues! I would like to send you observations of a new variable star (Brh V67), 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 V67 055805.2 +163901 (J2000) 11.2 11.5 (CCD) ? comments: Brh V67: GSC 1312 976 Comparison star was for all measurements GSC 1312 329 (11.2 mag), which was checked to be constant. GSC 1312 976 seems to have no entry in USNO A2.0 (?). A first data analysis using PDMWIN3.0 shows possible periods near 0.59,0.96 and 1.45 days, long period variability also cannot be excluded. object YYMMDD(UT) mag (CCD) code Brh V67 001221.0031 11.34 Brh.BAV Brh V67 001222.9753 11.37 Brh.BAV Brh V67 001223.9690 11.31 Brh.BAV Brh V67 010114.9031 11.24 Brh.BAV Brh V67 010116.0051 11.22 Brh.BAV Brh V67 010118.9003 11.18 Brh.BAV Brh V67 010127.9940 11.34 Brh.BAV Brh V67 010210.8496 11.48 Brh.BAV Brh V67 010224.8357 11.29 Brh.BAV Brh V67 010227.8056 11.28 Brh.BAV Brh V67 010227.8347 11.29 Brh.BAV Brh V67 010227.8833 11.33 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.tripod.de/KlausBernhard/index.html