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[vsnet-newvar 873] New variable star MisV1083

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1083).

MisV1083
  R.A.  21h03m11s.96
  Decl. +49o10'59".7  (2000.0)
  Mag.  12.8-13.8C
  Type  SR?
= IRAS 21015+4859  21h03m12s.0 +49o10'58"  Ellipse:5x3"  P.A.:38  Flux(12):26.04  Flux(25):16.14  Flux(60):2.634  Flux(100):<34.58  Var:99%

  http://vsnet.aerith.net/misao/data/MisV/MisV1083.gif

MisV1083 19990501.76068 13.38C Mis KAF-1600 - KenIchi_Kadota
MisV1083 19990501.76113 13.39C Mis KAF-1600 - KenIchi_Kadota
MisV1083 19990707.71403 13.78C Mis KAF-1600 - KenIchi_Kadota
MisV1083 19990707.71453 13.84C Mis KAF-1600 - KenIchi_Kadota
MisV1083 20000918.47298 12.79C Mis KAF-1600 - Nobuo_Ohkura
MisV1083 20000918.47485 12.76C Mis KAF-1600 - Nobuo_Ohkura
MisV1083 20000919.47598 12.86C Mis KAF-1600 - Nobuo_Ohkura
MisV1083 20001011.44720 12.99C Mis KAF-1600 - Nobuo_Ohkura
MisV1083 20001011.44907 12.94C Mis KAF-1600 - Nobuo_Ohkura
MisV1083 20001011.45092 13.03C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1083.

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 comparing with images taken by KenIchi Kadota, 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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