Vizier investigations reveal 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?285.8530_-03.7363 Here V-Ic information can be found showing a range of roughly +3.5 to +4, which is quite red, helping to confim it's LPV nature. Variation over long time intervals also appears to be of low amplitude with that extra data, so it is probably an Irregular LPV, though Semiregular is not precluded. Also in the MSX5C infrared catalogue. A more distant IRAS source could be just as easily associated with another similar mag star nearby. Cheers John John Greaves Klaus Bernhard wrote: > > Dear colleagues! > > I would like to send you observations of a new variable star > (Brh V115), 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 V115 190324.5 -034408 (J2000) 11.4-11.6 (CCD) > > comments: > Brh V115: GSC 5132 1538 > The comparison star is GSC 5136 1424 (12.0 mag), > which has been checked for constant brightness. > The USNO A2.0 magnitudes (r:10.9, b: 13.9) and > the following observations suggest a long period variable, > type and period still unknown. > > object YYMMDD(UT) mag(CCD) code > Brh V115 020627.0040 11.55 Brh.BAV > Brh V115 020629.0040 11.53 Brh.BAV > Brh V115 020629.9825 11.51 Brh.BAV > Brh V115 020630.9922 11.46 Brh.BAV > Brh V115 020701.9735 11.42 Brh.BAV > Brh V115 020705.9999 11.41 Brh.BAV > Brh V115 020707.9714 11.40 Brh.BAV > Brh V115 020708.9624 11.44 Brh.BAV > Brh V115 020719.9596 11.48 Brh.BAV > Brh V115 020720.9603 11.47 Brh.BAV > > Regards, > > Klaus Bernhard > > Klaus Bernhard > Kafkaweg 5 > A-4030 LINZ > AUSTRIA > > kl.bernhard@aon.at > http://mitglied.lycos.de/klausbernhard/ >