[vsnet-newvar 603] New variable star MisV1012

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1012).

MisV1012
  R.A.  20h01m41s.08
  Decl. +29o46'24".2  (2000.0)
  Mag.  12.8C-14.0C
  Type  SR:
= IRAS 19596+2937  R.A.=20 01 40.77  Decl.=+29 46 20.7  (25 x 4", p.a.=73)  flux(12)=1.38  flux(25)=0.87  flux(60)=<3.00  flux(100)=<60.88  90% variable
= 2MASS 200140.742 +294622.37 (2000.0)  8.109  6.859  6.114

  http://vsnet.aerith.net/misao/data/MisV/MisV1012.gif

MisV1012 19990430.69988 134C Mis image="KenIchi Kadota"
MisV1012 19990430.70034 134C Mis image="KenIchi Kadota"
MisV1012 19990707.68693 138C Mis image="KenIchi Kadota"
MisV1012 19990724.57868 140C Mis image="KenIchi Kadota"
MisV1012 19990801.60176 138C Mis image="KenIchi Kadota"
MisV1012 19990801.60219 139C Mis image="KenIchi Kadota"
MisV1012 19990831.63987 128C Mis image="KenIchi Kadota"
MisV1012 20000706.59704 137C Mis image="Nobuo Ohkura"
MisV1012 20000706.59889 133C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1012.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

The identification with the 2MASS data is by Taichi Kato.

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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