[vsnet-newvar 914] New variable star MisV1119

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1119).

MisV1119
  R.A.  21h25m59s.00
  Decl. +41o49'49".9  (2000.0)
  Mag.  11.8-12.9C
  Type  SR?
= USNO-A2.0 1275.15652812  21h25m59s.009 +41o49'49".85  Mag(R):15.6  Mag(B):19.6
= IRAS 21240+4136  21h25m59s.1 +41o49'48"  Ellipse:35x9"  P.A.:53  Flux(12):0.8113  Flux(25):0.3361  Flux(60):<0.4000  Flux(100):<12.97  Var:0%

  http://vsnet.aerith.net/misao/data/MisV/MisV1119.gif

MisV1119 20000907.51392 12.84C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20000907.51578 12.94C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20000907.51763 12.91C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20000926.47741 12.60C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20000926.47926 12.60C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20001106.39470 11.83C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20001106.39656 11.91C Mis KAF-1600 - Nobuo_Ohkura
MisV1119 20001106.39841 11.92C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1119.

It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
Nobuo Ohkura, and confirmed by KenIchi Kadota. 

The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.

The magnitude are measured automatically by the PIXY system 2.

About the MISAO Project and the PIXY system 2:
  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

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