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[vsnet-newvar 483] New variable star MisV0956

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0956).

MisV0956
  R.A.  19h07m31s.14
  Decl. +12o23'58".3  (2000.0)
  Mag.  13.4C-15.9C
  Type  M?
= IRAS 19051+1218  R.A.=19 07 28.10  Decl.=+12 23 42.9  (27 x 6", p.a.=79)  flux(12)=4.96  flux(25)=1.56  flux(60)=<0.62  flux(100)=<11.82  99% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0956.gif

MisV0956 19990723.50278 147C Mis image="KenIchi Kadota"
MisV0956 19990723.50424 150C Mis image="KenIchi Kadota"
MisV0956 19990723.51549 148C Mis image="KenIchi Kadota"
MisV0956 19990730.51487 151C Mis image="KenIchi Kadota"
MisV0956 19990730.52719 149C Mis image="KenIchi Kadota"
MisV0956 19990911.46961 155C Mis image="KenIchi Kadota"
MisV0956 19990911.47182 157C Mis image="KenIchi Kadota"
MisV0956 19990911.47602 159C Mis image="KenIchi Kadota"
MisV0956 20000401.71731 134C Mis image="KenIchi Kadota"
MisV0956 20000401.71811 134C Mis image="KenIchi Kadota"
MisV0956 20000401.71983 134C Mis image="KenIchi Kadota"
MisV0956 20000507.64259 141C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; and KenIchi Kadota, Ageo, Saitama,
Japan, discovered a new variable star MisV0956.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from 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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