[vsnet-newvar 437] New variable star MisV0919

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0919).

MisV0919
  R.A.  19h10m19s.48
  Decl. +12o34'01".1  (2000.0)
  Mag.  12.7C-15.3C
  Type  ?
= IRAS 19079+1228  R.A.=19 10 19.05  Decl.=+12 33 57.9  (29 x 8", p.a.=79)  flux(12)=2.02  flux(25)=0.99  flux(60)=<1.50  flux(100)=<14.57  97% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0919.gif

MisV0919 19990715.52338 128C Mis image="KenIchi Kadota"
MisV0919 19990715.52420 128C Mis image="KenIchi Kadota"
MisV0919 19990715.52759 128C Mis image="KenIchi Kadota"
MisV0919 19990715.52950 128C Mis image="KenIchi Kadota"
MisV0919 19990715.59178 129C Mis image="KenIchi Kadota"
MisV0919 19990715.59711 128C Mis image="KenIchi Kadota"
MisV0919 19990715.60150 128C Mis image="KenIchi Kadota"
MisV0919 19990715.60278 128C Mis image="KenIchi Kadota"
MisV0919 19990715.60579 127C Mis image="KenIchi Kadota"
MisV0919 20000507.64259 <142C Mis image="Nobuo Ohkura"
MisV0919 20000507.64444 153C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0919.

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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