[vsnet-newvar 527] New variable star MisV0978

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0978).

MisV0978
  R.A.  20h00m33s.25
  Decl. +22o43'41".2  (2000.0)
  Mag.  11.4C-12.3C
  Type  SR?
= GSC2141.1822  20 00 33.24  +22 43 41.3  14.14
= USNO-A2.0_1125.14870724  20 00 33.249  +22 43 41.17  13.0R  17.1B
= IRAS 19583+2235  R.A.=20 00 31.34  Decl.=+22 43 32.0  (46 x 8", p.a.=71)  flux(12)=0.48  flux(25)=<0.27  flux(60)=<0.40  flux(100)=<18.38

  http://vsnet.aerith.net/misao/data/MisV/MisV0978.gif

MisV0978 19990408.78207 119C Mis image="KenIchi Kadota"
MisV0978 19990430.70844 120C Mis image="KenIchi Kadota"
MisV0978 19990430.70888 120C Mis image="KenIchi Kadota"
MisV0978 19990601.64505 119C Mis image="KenIchi Kadota"
MisV0978 19990601.65907 119C Mis image="KenIchi Kadota"
MisV0978 19990724.57100 123C Mis image="KenIchi Kadota"
MisV0978 19990724.57144 123C Mis image="KenIchi Kadota"
MisV0978 20000606.58177 115C Mis image="Nobuo Ohkura"
MisV0978 20000606.58362 114C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0978.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

The identification with the 2MASS data is by Taichi Kato.

Please see the URL below for the MISAO Project and the PIXY system.

  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

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