Dear colleagues! I would like to send you observations of a new variable star (Brh V119), 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 V119 200504.1 -034035.8 (J2000) 11.5-11.7 (CCD) comments: Brh V119: GSC 5164 1289 The comparison star is GSC 5164 1327 (11.76 mag), which has been checked for constant brightness. The USNO A2.0 magnitudes (r:11.4, b: 14.0) and the following observations suggest a long period variable, type and period still unknown. object YYMMDD(UT) mag(CCD) code Brh V119 020627.0468 11.48 Brh.BAV Brh V119 020630.0253 11.58 Brh.BAV Brh V119 020701.0350 11.54 Brh.BAV Brh V119 020702.0163 11.52 Brh.BAV Brh V119 020706.0426 11.61 Brh.BAV Brh V119 020708.0142 11.62 Brh.BAV Brh V119 020720.0024 11.70 Brh.BAV Brh V119 020721.0031 11.69 Brh.BAV Vizier investigations show that further photometry for this object can be found via the TASS Mk III tenxcat database at: http://a188-l009.rit.edu/cgi-bin/tass_curve2.cgi?301.2670_-03.6767 These observations confirm the variability of GSC 5164 1289. Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.lycos.de/klausbernhard/