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[vsnet-campaign-dn 3567] Re: V601 Sco brightening?
- Date: Sat, 5 Apr 2003 11:05:55 +1000
- To: "Patrick Schmeer" <extpasc@rz.uni-saarland.de>,<vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp>,<vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp>
- From: "Rod Stubbings" <stubbo@sympac.com.au>
- Subject: [vsnet-campaign-dn 3567] Re: V601 Sco brightening?
- Delivered-To: vsnet-campaign-dn-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- References: <00c101c2facf$eac2bb80$74fd38cb@v9a8r1> <20030404182001.GA47125672@mars.rz.uni-saarland.de>
- Sender: owner-vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
> I wonder what star Rod observed - maybe the very red star 6" WNW of the
star
> marked on the Downes et al. finding chart (see the comments below)?
>
> I have three recent unfiltered CCD images of this field. On Mar. 13.484 UT
> this very red star had been as bright as on Mar. 9.488, but by Mar. 25.393
> it had faded considerably.
Patrick is correct - the red star 6" WNW has brighteded. I was hoping
someone was able to take some CCD images to show the variation. If the real
V601 Sco still exists we have two variables within 6". Is there a name for
this red star to report further observations ?
Regards,
Rod.
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