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[vsnet-newvar 888] New variable star MisV1093

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1093).

MisV1093
  R.A.  19h50m20s.77
  Decl. +36o11'09".8  (2000.0)
  Mag.  11.2-11.9C
  Type  ?
= USNO-A2.0 1200.13437934  19h50m20s.709 +36o11'09".43  Mag(R):14.4  Mag(B):17.6
= IRAS 19485+3603  19h50m20s.7 +36o11'10"  Ellipse:31x9"  P.A.:68  Flux(12):1.022  Flux(25):0.5340  Flux(60):<0.4998  Flux(100):<5.814  Var:5%
= 2MASS 195020.716 +361109.26 (2000.0)  6.576  5.590  5.074

  http://vsnet.aerith.net/misao/data/MisV/MisV1093.gif

MisV1093 19990803.64247 11.86C Mis KAF-1600 - KenIchi_Kadota
MisV1093 19990803.64291 11.90C Mis KAF-1600 - KenIchi_Kadota
MisV1093 20000920.43079 11.22C Mis KAF-1600 - Nobuo_Ohkura
MisV1093 20000920.43264 11.22C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1093.

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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