[vsnet-newvar 436] New variable star MisV0918

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0918).

MisV0918
  R.A.  19h09m13s.96
  Decl. +12o06'49".0  (2000.0)
  Mag.  12.9C-15.0C
  Type  ?
= IRAS 19068+1201  R.A.=19 09 13.46  Decl.=+12 06 47.3  (59 x 7", p.a.=79)  flux(12)=1.03  flux(25)=0.61  flux(60)=<1.86  flux(100)=<18.20  1% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0918.gif

MisV0918 19990715.52338 130C Mis image="KenIchi Kadota"
MisV0918 19990715.52420 131C Mis image="KenIchi Kadota"
MisV0918 19990715.52759 130C Mis image="KenIchi Kadota"
MisV0918 19990715.52950 130C Mis image="KenIchi Kadota"
MisV0918 19990715.59178 130C Mis image="KenIchi Kadota"
MisV0918 19990715.59711 130C Mis image="KenIchi Kadota"
MisV0918 19990715.60150 129C Mis image="KenIchi Kadota"
MisV0918 19990715.60278 130C Mis image="KenIchi Kadota"
MisV0918 19990715.60579 130C Mis image="KenIchi Kadota"
MisV0918 19990724.49234 131C Mis image="KenIchi Kadota"
MisV0918 19990724.49821 132C Mis image="KenIchi Kadota"
MisV0918 20000505.69694 149C Mis image="Nobuo Ohkura"
MisV0918 20000505.69878 150C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0918.

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/

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