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[vsnet-alert 5882] TAV J1907+117 not TAV J1907+171
- Date: Thu, 17 May 2001 18:44:32 +0100
- To: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- From: Guy M Hurst <guy@tahq.demon.co.uk>
- Subject: [vsnet-alert 5882] TAV J1907+117 not TAV J1907+171
- Cc: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign@kusastro.kyoto-u.ac.jp, vsnet-newvar@kusastro.kyoto-u.ac.jp
- In-Reply-To: <200105170505.OAA25983@rcsvr.rc.kyushu-u.ac.jp>
- References: <200105170505.OAA25983@rcsvr.rc.kyushu-u.ac.jp>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
In message <200105170505.OAA25983@rcsvr.rc.kyushu-u.ac.jp>, Hitoshi
YAMAOKA <yamaoka@rc.kyushu-u.ac.jp> writes
>Dear all,
>
>>According to H. Yamaoka (Kyushu University), the nearest brightest
>>star on DSS has an r=15.7, b=18.8, which suggests the variable is a
>>large-amplitude one.
>
>It is an USNO_A2.0 cataloged star, whose coordinate is: 19:07:27.055,
>+11:44:09.89. The r and b magnitudes are taken from USNO_A2.0. The
>USNO_A1.0 catalog does not contain this star.
>
>Sincerely Yours,
>Hitoshi Yamaoka, Kyushu Univ., Japan
>yamaoka@rc.kyushu-u.ac.jp
Dear Colleagues,
Please note the object announced on The Astronomer E-Circular 1633 and
now updated on 1634 today is designated TAV J1907+117 and not J1907+171
as in the subject line of your message circulating via VSNET.
Kind regards,
Guy Hurst
Editor, The Astronomer
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