[vsnet-newvar 825] New variable star MisV1068

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1068).

MisV1068
  R.A.  05h58m11s.37
  Decl. +23o06'14".1  (2000.0)
  Mag.  9.9-11.4C
  Type  SR:
= USNO-A2.0 1125.03089603  05h58m11s.435 +23o06'14".02  Mag(R):14.1  Mag(B):19.0
= IRAS 05551+2305  05h58m10s.8 +23o06'14"  Ellipse:28x6"  P.A.:90  Flux(12):7.209  Flux(25):5.514  Flux(60):0.7257  Flux(100):<8.437  Var:18%
= 2MASS 055811.460 +230613.57 (2000.0)  5.880  0.000  0.000

  http://vsnet.aerith.net/misao/data/MisV/MisV1068.gif

MisV1068 19990927.79100 11.07C Mis KAF-1600 - KenIchi_Kadota
MisV1068 19990927.79143 11.09C Mis KAF-1600 - KenIchi_Kadota
MisV1068 19991116.75531 11.39C Mis KAF-1600 - KenIchi_Kadota
MisV1068 19991116.75573 11.41C Mis KAF-1600 - KenIchi_Kadota
MisV1068 20000226.56188 9.86C Mis KAF-1600 - Nobuo_Ohkura
MisV1068 20000226.56373 9.94C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1068.

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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