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[vsnet-newvar 1021] New variable star MisV1135

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1135).

MisV1135
  R.A.  21h25m54s.85
  Decl. +49o40'42".6  (2000.0)
  Mag.  12.6-13.4C
  Type  SR?
= USNO-A2.0 1350.14054140  21h25m54s.783 +49o40'42".91  Mag(R):15.2  Mag(B):19.6
= IRAS 21241+4927  21h25m55s.1 +49o40'45"  Ellipse:16x9"  P.A.:47  Flux(12):0.7141  Flux(25):0.3170  Flux(60):<0.5780  Flux(100):<17.32  Var:23%
= 2MASS 212554.837 +494042.33 (2000.0)  7.835  6.394  5.742

  http://vsnet.aerith.net/misao/data/MisV/MisV1135.gif

MisV1135 19990709.67729 13.41C Mis KAF-1600 - KenIchi_Kadota
MisV1135 19990709.67786 13.36C Mis KAF-1600 - KenIchi_Kadota
MisV1135 20000918.48598 12.58C Mis KAF-1600 - Nobuo_Ohkura
MisV1135 20000918.48783 12.76C Mis KAF-1600 - Nobuo_Ohkura
MisV1135 20001013.45812 12.88C Mis KAF-1600 - Nobuo_Ohkura
MisV1135 20001013.45997 12.86C Mis KAF-1600 - Nobuo_Ohkura
MisV1135 20001013.46182 12.79C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1135.

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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