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[vsnet-newvar 817] New variable star MisV1060

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1060).

MisV1060
  R.A.  20h33m25s.15
  Decl. +31o50'34".3  (2000.0)
  Mag.  10.3-11.2C
  Type  ?
= USNO-A2.0 1200.15320568  20h33m25s.105 +31o50'34".74  Mag(R):14.1  Mag(B):17.7
= IRAS 20314+3140  20h33m26s.6 +31o50'43"  Ellipse:22x3"  P.A.:68  Flux(12):1.072  Flux(25):0.4573  Flux(60):<0.6813  Flux(100):<32.65  Var:19%

  http://vsnet.aerith.net/misao/data/MisV/MisV1060.gif

MisV1060 19990605.74300 11.16C Mis KAF-1600 - KenIchi_Kadota
MisV1060 19990605.74347 11.23C Mis KAF-1600 - KenIchi_Kadota
MisV1060 20000709.59055 10.25C Mis KAF-1600 - Nobuo_Ohkura
MisV1060 20000709.59240 10.29C Mis KAF-1600 - Nobuo_Ohkura
MisV1060 20000716.59352 10.33C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1060.

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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