[vsnet-newvar 472] New variable star MisV0945

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0945).

MisV0945
  R.A.  19h07m50s.30
  Decl. +12o50'44".9  (2000.0)
  Mag.  12.8C-16.5C
  Type  M:
= USNO-A2.0_0975.14166390  19 07 50.300  +12 50 44.92  13.6R  17.2B

  http://vsnet.aerith.net/misao/data/MisV/MisV0945.gif

MisV0945 19990715.52338 164C Mis image="KenIchi Kadota"
MisV0945 19990715.52420 158C Mis image="KenIchi Kadota"
MisV0945 19990715.52759 156C Mis image="KenIchi Kadota"
MisV0945 19990715.52950 165C Mis image="KenIchi Kadota"
MisV0945 19990715.59178 160C Mis image="KenIchi Kadota"
MisV0945 19990715.60150 165C Mis image="KenIchi Kadota"
MisV0945 19990715.60278 162C Mis image="KenIchi Kadota"
MisV0945 19990715.60579 156C Mis image="KenIchi Kadota"
MisV0945 19990724.49234 158C Mis image="KenIchi Kadota"
MisV0945 19990724.49821 160C Mis image="KenIchi Kadota"
MisV0945 19990911.47602 144C Mis image="KenIchi Kadota"
MisV0945 20000401.71811 136C Mis image="KenIchi Kadota"
MisV0945 20000401.71983 136C Mis image="KenIchi Kadota"
MisV0945 20000507.64259 128C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0945.

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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