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[vsnet-newvar 889] New variable star MisV1094

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1094).

MisV1094
  R.A.  19h59m02s.30
  Decl. +36o20'06".3  (2000.0)
  Mag.  12.4-13.1C
  Type  SR:
= USNO-A2.0 1200.14049380  19h59m02s.186 +36o20'05".46  Mag(R):15.1  Mag(B):18.4
= 2MASS 195902.216 +362005.06 (2000.0)  8.382  7.285  6.775

  http://vsnet.aerith.net/misao/data/MisV/MisV1094.gif

MisV1094 19990430.69374 12.55C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990430.69417 12.59C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990707.67965 12.83C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990707.68009 12.87C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990801.61065 12.98C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990801.61109 13.03C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990803.65726 12.96C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990803.65770 13.11C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990831.63196 12.70C Mis KAF-1600 - KenIchi_Kadota
MisV1094 19990831.63242 12.77C Mis KAF-1600 - KenIchi_Kadota
MisV1094 20000920.43636 12.40C Mis KAF-1600 - Nobuo_Ohkura
MisV1094 20000920.43821 12.40C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1094.

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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