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[vsnet-alert 4001] KZ Gem(?) in rare outburst - confirmation and first analysis of CCD run
- Date: Mon, 10 Jan 2000 21:32:02 +0100
- To: <vsnet-alert@kusastro.kyoto-u.ac.jp>
- From: "Tonny Vanmunster" <Tonny.Vanmunster@advalvas.be>
- Subject: [vsnet-alert 4001] KZ Gem(?) in rare outburst - confirmation and first analysis of CCD run
- Importance: Normal
- In-Reply-To: <20000109194745.C6385@rz.uni-sb.de>
- Reply-To: <Tonny.Vanmunster@advalvas.be>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear all,
KZ Gem (or more precise: the object indicated by P. Schmeer) is indeed in outburst, as confirmed by my CCD observations of Jan 09/10, 2000, obtained at CBA Belgium Observatory. I have monitored the object using the 0.35-m f/6.3 telescope and a ST-7 CCD (unfiltered) for about 2.6 hours. The resulting light curve is quite flat, showing no periodic modulations.
2000 Jan 09.967 UT, mag 14.8 C
Best regards,
Tonny Vanmunster
CBA Belgium Observatory
> -----Original Message-----
> From: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
> [mailto:owner-vsnet-alert@kusastro.kyoto-u.ac.jp]On Behalf Of Patrick
> Schmeer
> Sent: zondag 9 januari 2000 19:48
> To: vsnet-alert@kusastro.kyoto-u.ac.jp; Patrick Schmeer
> Subject: [vsnet-alert 3991] KZ Gem(?) in rare outburst
>
>
> My alert message:
>
> KZ Gem appears to be in outburst at mag 14. Can you confirm?
>
>
> Rod Stubbings' reply:
>
> > Cannot confirm outburst. I've had this field under observation
> and didn't
> > notice any change tonight. After your message I went out to look at the
> > field again but could not see an outburst. I'm using the vsnet
> chart. The
> > last few nights I thought there might have been an outburst but
> to me the
> > close star above KZ Gem seems to have brightened a little.
>
>
> My reply:
>
> There are three USNO-A2.0 stars very close to the catalogued position of
> KZ Gem:
> A) 06:53:02.496 +16:40:05.96 14.3 15.3
> B) 06:53:02.468 +16:40:00.05 14.9 16.5
> C) 06:53:02.744 +16:39:50.61 17.6 17.9
>
> The star marked in DWS97 is just north of star C and southeast of B.
> Star B (or a very close companion of it) is the outbursting object. It
> brightened by 2 magnitudes since Jan. 7.302 UT and was as bright as
> star A (mag 14.3) on an unfiltered CCD image taken on Jan. 9.292 UT.
> I haven't yet received the original finding chart, but I would consider
> it as highly unlikely that there are two outbursting objects so close
> together (both reaching mag 14). It's much more likely that the wrong
> star is marked in DWS97.
>
> According to the GCVS KZ Gem is a dwarf nova with a photographic
> magnitude range of 14.7-[18.5 and a mean cycle length of 258 days.
>
> Astrometry, spectroscopy, and high-speed photometry during the current
> rare outburst are very urgently required.
>
> Patrick
>
> P.S.:
> Please forget about CW Mon and turn your attention to this star (if
> still bright) - or RX J0640-24.
>
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