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[vsnet-alert 5728] Re: Possible Nova in Saggitarius; astrometry and the quiescent counterpart
- Date: Mon, 26 Feb 2001 09:02:25 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@kusastro.kyoto-u.ac.jp, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-alert 5728] Re: Possible Nova in Saggitarius; astrometry and the quiescent counterpart
- Cc: green@cfa.harvard.edu, kenic-k@astroarts.co.jp
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear all,
>Immediately neighbourhood of this position, an USNO_A2.0 star
>(position end figures 40s.414, 15".40, rmag = 15.8, bmag = 17.4)
>exists, which is the plausible counterpart at quiescent.
This star is really seen on DSS2R image. There seems to exist an dim
(rmag about 18) star 2"-3" northeast of this USNO star, and no other
object can be seen in 5" radius.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
Return to Daisaku Nogami
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