[vsnet-newvar 488] New variable star MisV0961

[Seiichi Yoshida <comet@aerith.net>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0961).

MisV0961
  R.A.  19h01m36s.85
  Decl. +00o47'08".8  (2000.0)
  Mag.  12.6C-13.6C
  Type  ?
= IRAS 18590+0042  R.A.=19 01 36.88  Decl.=+00 47 08.8  (19 x 4", p.a.=50)  flux(12)=3.14  flux(25)=1.31  flux(60)=<11.06  flux(100)=<139.20  72% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV0961.gif

MisV0961 19990220.84734 <122C Mis image="KenIchi Kadota"
MisV0961 19990220.84824 <122C Mis image="KenIchi Kadota"
MisV0961 19990220.84925 <124C Mis image="KenIchi Kadota"
MisV0961 19990220.85015 <124C Mis image="KenIchi Kadota"
MisV0961 19990429.72848 135C Mis image="KenIchi Kadota"
MisV0961 19990429.72892 136C Mis image="KenIchi Kadota"
MisV0961 19990707.64562 128C Mis image="KenIchi Kadota"
MisV0961 19990707.64606 129C Mis image="KenIchi Kadota"
MisV0961 20000503.61328 126C Mis image="Nobuo Ohkura"
MisV0961 20000503.61513 127C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0961.

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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