[vsnet-newvar 893] New variable star MisV1098

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1098).

MisV1098
  R.A.  20h09m39s.15
  Decl. +36o05'49".2  (2000.0)
  Mag.  13.2-14.1C
  Type  ?
= IRAS 20077+3556  20h09m39s.5 +36o05'46"  Ellipse:30x3"  P.A.:61  Flux(12):0.6270  Flux(25):0.4284  Flux(60):<4.303  Flux(100):<38.92  Var:19%
= 2MASS 200939.167 +360549.20 (2000.0)  7.903  6.505  5.897

  http://vsnet.aerith.net/misao/data/MisV/MisV1098.gif

MisV1098 19990803.68073 14.10C Mis KAF-1600 - KenIchi_Kadota
MisV1098 19990803.68119 13.96C Mis KAF-1600 - KenIchi_Kadota
MisV1098 19991121.41226 13.39C Mis KAF-1600 - KenIchi_Kadota
MisV1098 19991121.41269 13.45C Mis KAF-1600 - KenIchi_Kadota
MisV1098 20000920.44193 13.31C Mis KAF-1600 - Nobuo_Ohkura
MisV1098 20000920.44378 13.18C Mis KAF-1600 - Nobuo_Ohkura
MisV1098 20000920.44563 13.17C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1098.

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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