[vsnet-newvar 905] New variable star MisV1110

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1110).

MisV1110
  R.A.  20h45m43s.17
  Decl. +44o00'44".1  (2000.0)
  Mag.  13.3-15.7C
  Type  M?
= USNO-A2.0 1275.14115474  20h45m43s.179 +44o00'37".67  Mag(R):17.3  Mag(B):18.2
= 2MASS 204543.119 +440044.51 (2000.0)  8.309  6.865  6.054

  http://vsnet.aerith.net/misao/data/MisV/MisV1110.gif

MisV1110 20000803.54463 15.35C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20000803.54649 15.41C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20000803.54835 15.71C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20000905.48153 14.15C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20000905.48337 14.25C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20001001.46106 13.29C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20001001.46292 13.41C Mis KAF-1600 - Nobuo_Ohkura
MisV1110 20001001.46477 13.42C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1110.

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, 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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