[vsnet-newvar 602] New variable star MisV1011

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1011).

MisV1011
  R.A.  19h57m41s.93
  Decl. +29o44'38".7  (2000.0)
  Mag.  12.6C-14.4C
  Type  SR?
= IRAS 19556+2936  R.A.=19 57 41.68  Decl.=+29 44 36.5  (25 x 6", p.a.=73)  flux(12)=1.13  flux(25)=0.49  flux(60)=<0.67  flux(100)=<39.68  0% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV1011.gif

MisV1011 19990430.69988 141C Mis image="KenIchi Kadota"
MisV1011 19990430.70034 142C Mis image="KenIchi Kadota"
MisV1011 19990707.68650 130C Mis image="KenIchi Kadota"
MisV1011 19990707.68693 130C Mis image="KenIchi Kadota"
MisV1011 19990724.57868 130C Mis image="KenIchi Kadota"
MisV1011 19990724.57913 129C Mis image="KenIchi Kadota"
MisV1011 19990801.60176 129C Mis image="KenIchi Kadota"
MisV1011 19990801.60219 130C Mis image="KenIchi Kadota"
MisV1011 19990831.63987 126C Mis image="KenIchi Kadota"
MisV1011 20000706.59519 143C Mis image="Nobuo Ohkura"
MisV1011 20000706.59704 144C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1011.

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".

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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