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[vsnet-newvar 857] New variable star MisV1078

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1078).

MisV1078
  R.A.  20h39m29s.17
  Decl. +49o04'52".2  (2000.0)
  Mag.  11.0-11.8C
  Type  SR?
= USNO-A2.0 1350.12707492  20h39m29s.225 +49o04'51".79  Mag(R):13.0  Mag(B):16.6
= IRAS 20379+4854  20h39m29s.0 +49o04'52"  Ellipse:16x10"  P.A.:140  Flux(12):0.7670  Flux(25):<0.3901  Flux(60):<0.8116  Flux(100):<38.36

  http://vsnet.aerith.net/misao/data/MisV/MisV1078.gif

MisV1078 19990709.75131 11.52C Mis KAF-1600 - KenIchi_Kadota
MisV1078 19990709.75178 11.55C Mis KAF-1600 - KenIchi_Kadota
MisV1078 19991121.46025 11.73C Mis KAF-1600 - KenIchi_Kadota
MisV1078 19991121.46069 11.84C Mis KAF-1600 - KenIchi_Kadota
MisV1078 20000919.45744 11.34C Mis KAF-1600 - Nobuo_Ohkura
MisV1078 20001011.43238 10.97C Mis KAF-1600 - Nobuo_Ohkura
MisV1078 20001011.43423 11.02C Mis KAF-1600 - Nobuo_Ohkura
MisV1078 20001011.43609 11.05C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1078.

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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