Dear
colleagues!
I would like to send you observations of a new variable star (Brh V117), 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 V117 184231.48 -033539.6 (J2000) 12.5-12.8 (CCD) comments: Brh V117: GSC 2.2 S300313115612 The comparison star is GSC 5117 2186 (12.6 mag), which has been checked for constant brightness. The GSC 2.2 magnitudes (r:11.7, b: 15.2) and the following observations suggest a long period variable, type and period still unknown. 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_curve.cgi?11945383_280.6312_-3.5943 These observations confirm the variability of this object. object YYMMDD(UT) mag(CCD) code BrhV117 020626.9895 12.82 Brh.BAV BrhV117 020628.9895 12.82 Brh.BAV BrhV117 020629.9680 12.79 Brh.BAV BrhV117 020630.9777 12.76 Brh.BAV BrhV117 020701.9590 12.75 Brh.BAV BrhV117 020705.9854 12.72 Brh.BAV BrhV117 020707.9569 12.72 Brh.BAV BrhV117 020708.9479 12.71 Brh.BAV BrhV117 020719.9451 12.61 Brh.BAV BrhV117 020720.9458 12.55 Brh.BAV Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.lycos.de/klausbernhard/ |