Dear Prof. Samus, > I have a question concerning your paper "The 1995 Outburst of DV Dra" > (IBVS, 1995, No. 4279). In the paper, you quote the coordinates of the > star (18h17m24s.44 +50deg48'16".6, 2000) you report to have been observed > in a new outburst. We possess the discovery plates used by Pavlov and > Shugarov (Astron. Tsirk., 1985, No. 1373), clearly showing DV Dra in > outburst at a position different from yours; our photographic astrometry > of DV Dra gives the coordinates 18h17m23s.10 +50deg48'18".08, 2000.0, ep. > 1984.433. Your VSNET light curve clearly shows variations. Either you > observe another star, or your published position is in error. Can you > kindly comment? The matter had been discussed in vsnet-id 182 and 183 (attached below). Now it is evident that the true DV Dra is different from that reported in IBVS 4279. The most likely explanation is that the detected object (not DV Dra) is a red star, which appeared bright on Iida's unfiltered CCD images. He made many negative observations in 1994 and 1995, but they did not reach the detection magnitude. It looks most likely this star is at the very limit of Iida's system, which made a transient positive detection. The two V-band observations made at Ouda Station both showed V=18.6 (as mentioned in IBVS 4279), which are consistent with the likely conclusion that this star did not vary very significantly. The single Ouda magnitude quoted in the VSNET observations (VSNET light curve) doesn't seem to correctly reflect the published magnitude. (The on-line light curve incorrectly referes to vsnet-obs 1595, which was superseded by vsnet-obs 1605; I will correct this error and incorrect Iida's entries). In conclusion, ther was no true DV Dra outburst in 1995 October-November. Regards, Taichi Kato --- Subject: [vsnet-id 182] (fwd) On DV Dra identification (fwd) On DV Dra identification Date: Sun, 7 May 2000 20:51:36 +0300 (EET DST) From: stars@personal.eunet.fi (Timo Kinnunen) Subject: DV Dra id problem Hello, In the following message Kato-San wrote: >[vsnet-obs 1605] DV Dra outburst, continuing? > >DV Dra > > A 6-min V-band CCD exposure of DV Dra taken at Ouda Station last night >clearly shows DV Dra (WZ Sge-type candidate) siginificantly brighter than >in Downes & Shara (1993) chart. Astrometry using 6 GSC stars (mean residual >0".3) gives 18h17m24s.44 +50o48'16".6 (J2000.0). This position is slightly >different from that given in Downes & Shara (1993), but is in good agreement >with one (18h17m24s.44 +50o48'16".3) obtained by M. Iida from his outburst >CCD image (Iida, private communication). Reanalysis of the Nov. 13 CCD >image (already reported in vsnet-obs #1595, but the measurement was done >for the coordinates by Downes & Shara (1993)) confirms this finding. The position given above, and also the SIMBAD position: 18 17 25.070 +50 48 14.50 (2000) fall only a few arcseconds from an A2.0 star 1350.09592107 - at 18 17 24.71 +50 48 19.19 (2000) DV Dra can be very easily confused with this star - it is certainly noteworthy, however I could not find any remarks on it from 1995 outburst reports. Pardon me, I don't have the relevant IBVS issue at hand, but I find it interesting that the outburst photometry apparently was not disturbed by this A2.0 star. > Reexamination of POSS and the candidate by Downes & >Shara (1993) in digitized GSC survey plate would help identifying the nature >of this intriguing outburst. I checked the available POSS scans at USNO Flagstaff - the following plate shows a DV Dra candidate some 10" due N from this A2.0 star. Details: > POSSII 0229 SJ06278 1995.4976 see 5' square image at http://vsnet.nofs.navy.mil/tmp/fchaanCqa_sj0229.000.jpg I believe the date is close to 1995 June 30 - about four months prior to the outburst report by Iida, so it would be very intriguing to find out whether the POSS-II candidate is true DV Dra, another variable, or a plate flaw. Regards, Timo Kinnunen Subject: [vsnet-id 183] Re: (fwd) On DV Dra identification Re: (fwd) On DV Dra identification > DV Dra can be very easily confused with this star - it is > certainly noteworthy, however I could not find any remarks on it > from 1995 outburst reports. There was no USNO at that time, and we noticed, as already cited, a slight difference in position from Downes & Shara (1993). However, astrometry of both observations were done near the limiting magnitude. The question is still open whether the USNO star is different from or identical with the true DV Dra or the "outbursting object" in 1995. The chart in the original discovery announcement of DV Dra was not good enough to discriminate such a subtle difference. The second outburst report contained no chart. Regards, Taichi Kato