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[vsnet-newvar 434] New variable star MisV0916
- Date: Wed, 14 Jun 2000 20:26:56 -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 434] New variable star MisV0916
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0916).
MisV0916
R.A. 18h57m01s.78
Decl. +12o41'25".7 (2000.0)
Mag. 13.0C-<15.0C
Type M?
= IRAS 18547+1237 R.A.=18 57 01.46 Decl.=+12 41 23.9 (28 x 7", p.a.=79) flux(12)=0.82 flux(25)=0.56 flux(60)=<0.40 flux(100)=<3.82 12% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0916.gif
MisV0916 19990429.71339 144C Mis image="KenIchi Kadota"
MisV0916 19990429.71382 144C Mis image="KenIchi Kadota"
MisV0916 19990923.47565 <150C Mis image="KenIchi Kadota"
MisV0916 19990923.47610 <150C Mis image="KenIchi Kadota"
MisV0916 20000507.63334 132C Mis image="Nobuo Ohkura"
MisV0916 20000507.63520 130C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0916.
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