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[vsnet-obs 23999] New variable star MisV0508
- Date: Sat, 23 Oct 1999 17:44:45 +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 23999] New variable star MisV0508
- cc: seiichi@mura01.muraoka.info.waseda.ac.jp
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0508).
MisV0508
R.A. 18h41m03s.10
Decl. -28o09'35".6 (2000.0)
Mag. 11.5C-13.3C
Type ?
= GSC6870.1383 18 41 03.22 -28 09 35.7 12.68
= USNO-A2.0_0600.36532866 18 41 03.101 -28 09 35.61 12.0R 18.8B
= IRAS 18379-2812 R.A.=18 41 05.40 Decl.=-28 09 34.0 (73 x 10", p.a.=87) flux(12)=0.49 flux(25)=<0.64 flux(60)=<0.40 flux(100)=<2.92
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/data/MisV/MisV0508.gif
MisV0508 19990715.58696 115C Mis
MisV0508 19990715.58741 115C Mis
MisV0508 19990715.58797 116C Mis
MisV0508 19990923.44294 133C Mis
It was detected by the PIXY system as one of the candidates of new
variable stars from images taken by KenIchi Kadota, Ageo City,
Saitama, Japan, then confirmed by Seiichi Yoshida.
This object and V949 Sgr, a nova in 1914, are at the same position
within 12 arcsec. Maybe it is a recurrent nova or the nova in 1914 was
just a red variable.
Please see the URL below for the MISAO Project and the PIXY system.
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/
--
Seiichi Yoshida
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp