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[vsnet-newvar 448] New variable star MisV0930
- Date: Wed, 14 Jun 2000 21:52:38 -0500
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.su, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 448] New variable star MisV0930
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0930).
MisV0930
R.A. 19h41m03s.13
Decl. +15o34'18".6 (2000.0)
Mag. 12.8C-<14.8C
Type ?
= IRAS 19387+1527 R.A.=19 41 03.01 Decl.=+15 34 15.2 (16 x 4", p.a.=72) flux(12)=6.48 flux(25)=7.74 flux(60)=1.43 flux(100)=<2.72 99% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0930.gif
MisV0930 19990715.61795 <148C Mis image="KenIchi Kadota"
MisV0930 19990715.61840 <148C Mis image="KenIchi Kadota"
MisV0930 19990715.63223 <148C Mis image="KenIchi Kadota"
MisV0930 19990715.63291 <148C Mis image="KenIchi Kadota"
MisV0930 20000509.63321 128C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0930.
It was detected by the PIXY system as one of the candidates of new
variable stars from images taken by Ohkura comparing with images taken
by Kadota, then confirmed by Yoshida.
The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".
Please see the URL below for the MISAO Project and the PIXY system.
http://vsnet.aerith.net/misao/
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp