[vsnet-newvar 1022] New variable star MisV1136

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1136).

MisV1136
  R.A.  21h29m55s.28
  Decl. +49o27'53".7  (2000.0)
  Mag.  13.4-15.9C
  Type  M?
= IRAS 21281+4914  21h29m55s.4 +49o27'52"  Ellipse:60x12"  P.A.:50  Flux(12):0.2550  Flux(25):<0.2500  Flux(60):<0.4480  Flux(100):<18.74
= 2MASS 212955.274 +492753.90 (2000.0)  8.898  7.700  7.047

  http://vsnet.aerith.net/misao/data/MisV/MisV1136.gif

MisV1136 19990709.67729 13.47C Mis KAF-1600 - KenIchi_Kadota
MisV1136 19990709.67786 13.44C Mis KAF-1600 - KenIchi_Kadota
MisV1136 20000805.56452 <15.14C Mis KAF-1600 - Nobuo_Ohkura
MisV1136 20000918.48968 15.85C Mis KAF-1600 - Nobuo_Ohkura
MisV1136 20000918.49154 15.57C Mis KAF-1600 - Nobuo_Ohkura
MisV1136 20001013.45997 15.65C Mis KAF-1600 - Nobuo_Ohkura
MisV1136 20001013.46182 15.59C Mis KAF-1600 - Nobuo_Ohkura
MisV1136 20001013.46367 15.33C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1136.

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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