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[vsnet-newvar 1370] New variable star MisV1152

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1152).

MisV1152
  R.A.  20h32m30s.60
  Decl. +49o36'38".0  (2000.0)
  Mag.  11.9-12.9C
  Type  SR?
= USNO-A2.0 1350.12520383  20h32m30s.652 +49o36'38".21  Mag(R):14.9  Mag(B):19.6
= IRAS 20309+4926  20h32m30s.4 +49o36'37"  Ellipse:30x5"  P.A.:57  Flux(12):2.068  Flux(25):0.9527  Flux(60):<1.241  Flux(100):<9.973  Var:8%
= MSX5C G086.8454+05.8044  20h32m30s.67 +49o36'36".4  InScanError:3.1"  CrossScanError:2.4"  Flux(A):2.4385  Flux(C):1.8607  Flux(D):1.7985

  http://vsnet.aerith.net/misao/data/MisV/MisV1152.gif

MisV1152 20000919.45372 11.91C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20000919.45557 11.87C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20001013.42473 12.30C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20001013.42657 12.32C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20001013.42845 12.39C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20011003.44258 12.86C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20011003.44455 12.84C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1152 20011003.44652 12.80C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1152.

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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