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[vsnet-newvar 438] New variable star MisV0920

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0920).

MisV0920
  R.A.  19h10m17s.18
  Decl. +12o52'39".6  (2000.0)
  Mag.  12.5C-<14.8C
  Type  ?
= IRAS 19079+1247  R.A.=19 10 16.69  Decl.=+12 52 32.7  (27 x 9", p.a.=79)  flux(12)=2.33  flux(25)=1.06  flux(60)=<1.31  flux(100)=<13.58  80% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0920.gif

MisV0920 19990715.52338 <148C Mis image="KenIchi Kadota"
MisV0920 19990715.52420 <148C Mis image="KenIchi Kadota"
MisV0920 19990715.52759 <144C Mis image="KenIchi Kadota"
MisV0920 19990715.52950 <148C Mis image="KenIchi Kadota"
MisV0920 19990715.59178 <146C Mis image="KenIchi Kadota"
MisV0920 19990715.59711 <145C Mis image="KenIchi Kadota"
MisV0920 19990715.60150 <147C Mis image="KenIchi Kadota"
MisV0920 19990715.60278 <148C Mis image="KenIchi Kadota"
MisV0920 19990715.60579 <148C Mis image="KenIchi Kadota"
MisV0920 20000507.64259 126C Mis image="Nobuo Ohkura"
MisV0920 20000507.64444 125C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0920.

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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