[vsnet-newvar 489] New variable star MisV0962

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0962).

MisV0962
  R.A.  19h24m29s.65
  Decl. +04o56'39".5  (2000.0)
  Mag.  11.4C-12.9C
  Type  SR?
= USNO-A2.0_0900.14935700  19 24 29.653  +04 56 39.49  15.0R  18.7B
= IRAS 19220+0450  R.A.=19 24 29.58  Decl.=+04 56 37.1  (26 x 7", p.a.=79)  flux(12)=0.90  flux(25)=0.38  flux(60)=<0.40  flux(100)=<17.64  23% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0962.gif

MisV0962 20000216.82586 115C Mis image="KenIchi Kadota"
MisV0962 20000216.82875 114C Mis image="KenIchi Kadota"
MisV0962 20000216.83083 115C Mis image="KenIchi Kadota"
MisV0962 20000308.79802 117C Mis image="KenIchi Kadota"
MisV0962 20000319.82475 118C Mis image="KenIchi Kadota"
MisV0962 20000319.82718 119C Mis image="KenIchi Kadota"
MisV0962 20000401.71226 120C Mis image="KenIchi Kadota"
MisV0962 20000401.71418 119C Mis image="KenIchi Kadota"
MisV0962 20000523.62686 129C Mis image="Nobuo Ohkura"
MisV0962 20000523.62872 127C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0962.

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".

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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