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[vsnet-id 378] R: [vsnet-chat 4023] Re: Object Near GSC 770
- Date: Mon, 22 Jan 2001 14:07:23 +0100
- To: "Hitoshi YAMAOKA" <yamaoka@rc.kyushu-u.ac.jp>, <vsnet-chat@kusastro.kyoto-u.ac.jp>, <vsnet-id@kusastro.kyoto-u.ac.jp>
- From: "Toni Scarmato" <toniscarmato@hotmail.com>
- Subject: [vsnet-id 378] R: [vsnet-chat 4023] Re: Object Near GSC 770
- References: <200101221023.TAA08063@rcsvr.rc.kyushu-u.ac.jp>
- Sender: owner-vsnet-id@kusastro.kyoto-u.ac.jp
Dear Hitoshi, Taichi and Patrick.
Thanks very much for your comment.
I Am searching in my photografic archive because I think that I Have other
images of the same field at the time 2000/06/19-25.
More informations at the next e-mail.
Regards,
Toni Scarmato
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----- Original Message -----
From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
To: <vsnet-chat@kusastro.kyoto-u.ac.jp>; <vsnet-id@kusastro.kyoto-u.ac.jp>
Cc: <toniscarmato@hotmail.com>
Sent: Monday, January 22, 2001 11:23 AM
Subject: [vsnet-chat 4023] Re: Object Near GSC 770
> > The object is rather securely identified with the following 2MASS
> >star.
> >
> >2MASS 173642.178 -234916.19 (2000.0) 9.225 8.067 7.569
>
> It is the identification for V2220 Oph.
>
> > Furthermore, there is a NSV star (NSV09220) even closer (but
> >apparently different) to Toni's suspected stellar image.
>
> NSV 9200 is also referred by Terzan and Rutily, 1972, A&Ap, 16, 408,
> Fig. 4 as star 10. It is definetely not the Toni's suspected.
>
> There is only one information that star "A" can be a variable:
> somewhat bright r magnitude on USNO_A2.0 but apparently dimmer on DSS2
> R image.
>
> Sincerely Yours,
> Hitoshi Yamaoka, Kyushu Univ., Japan
> yamaoka@rc.kyushu-u.ac.jp
>
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