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[vsnet-obs 24836] Re: New variable star MisV0314
- Date: Tue, 23 Nov 1999 19:11:02 +0900
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.su, vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <seiichi@muraoka.info.waseda.ac.jp>
- Subject: [vsnet-obs 24836] Re: New variable star MisV0314
- cc: seiichi@mura01.muraoka.info.waseda.ac.jp
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Dear colleagues,
Here is the corrigendum on the discovery announcement of MisV0314 on
Sept. 1, 1999.
> V1191 Oph is 66.5 arcsec from MisV0314. No star brighter than 15.3C
> mag was detected at the position of V1191 Oph. However, considering
> the large distance, MisV0314 is probably another new variable object.
should be:
V1191 Oph is 1.2 arcmin from MisV0314, that was detectec on Kadota's
unfiltered CCD images as a 13 mag star. MisV0314 is thus another new
variable star.
Best regards,
--
Seiichi Yoshida
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html
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