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[vsnet-newvar 886] New variable star MisV1091

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1091).

MisV1091
  R.A.  19h59m31s.97
  Decl. +35o34'45".6  (2000.0)
  Mag.  13.2-14.6C
  Type  SR?
= USNO-A2.0 1200.14081434  19h59m32s.013 +35o34'45".47  Mag(R):16.9  Mag(B):18.9
= 2MASS 195931.959 +353446.04 (2000.0)  8.351  7.275  6.737

  http://vsnet.aerith.net/misao/data/MisV/MisV1091.gif

MisV1091 19990430.69374 14.26C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990430.69417 14.01C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990707.67965 14.20C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990707.68009 14.63C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990801.61065 13.61C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990801.61109 13.56C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990803.65726 13.61C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990803.65770 13.41C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990831.63196 13.26C Mis KAF-1600 - KenIchi_Kadota
MisV1091 19990831.63242 13.15C Mis KAF-1600 - KenIchi_Kadota

Seiichi Yoshida, MISAO Project; and KenIchi Kadota, Ageo, Saitama,
Japan, discovered a new variable star MisV1091.

It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from 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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