[vsnet-newvar 877] New variable star MisV1087

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1087).

MisV1087
  R.A.  21h14m45s.02
  Decl. +46o31'11".0  (2000.0)
  Mag.  12.4-13.9C
  Type  SR:
= USNO-A2.0 1350.13714462  21h14m45s.056 +46o31'13".64  Mag(R):14.5  Mag(B):18.6
= IRAS 21129+4618  21h14m42s.5 +46o30'46"  Ellipse:80x9"  P.A.:52  Flux(12):0.3369  Flux(25):<0.2500  Flux(60):<0.5398  Flux(100):<21.46
= 2MASS 211445.028 +463110.88 (2000.0)  8.758  7.518  6.844

  http://vsnet.aerith.net/misao/data/MisV/MisV1087.gif

MisV1087 19991121.51011 13.58C Mis KAF-1600 - KenIchi_Kadota
MisV1087 19991121.51125 13.26C Mis KAF-1600 - KenIchi_Kadota
MisV1087 20000804.55922 13.73C Mis KAF-1600 - Nobuo_Ohkura
MisV1087 20000804.56107 13.86C Mis KAF-1600 - Nobuo_Ohkura
MisV1087 20000804.56292 13.89C Mis KAF-1600 - Nobuo_Ohkura
MisV1087 20001009.45928 12.42C Mis KAF-1600 - Nobuo_Ohkura
MisV1087 20001009.46112 12.45C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1087.

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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