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[vsnet-newvar 332] New variable star MisV0850

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0850).

MisV0850
  R.A.  18h02m03s.69
  Decl. -32o38'32".7  (2000.0)
  Mag.  12.8C-14.5C
  Type  ?
= IRAS 17588-3238  R.A.=18 02 05.73  Decl.=-32 38 37.0  (70 x 11", p.a.=92)  flux(12)=0.55  flux(25)=<0.78  flux(60)=<4.08  flux(100)=<41.08

  http://vsnet.aerith.net/misao/data/MisV/MisV0850.gif

MisV0850 19990520.68679 128C Mis
MisV0850 19990520.68723 128C Mis
MisV0850 20000224.84394 145C Mis
MisV0850 20000224.84450 141C Mis

It was detected by the PIXY system as one of the candidates of new
variable stars from images taken by KenIchi Kadota, Ageo City,
Saitama, Japan, then confirmed by Seiichi Yoshida.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis", except for ones taken by
KenIchi Kadota.

NSV 09990 is 2.6 arcmin from MisV0850. No star brighter than 14.5 mag
was detected at the cataloged position of NSV 09990. But considering
the large angular distance and the magnitude of NSV 09990 (15.3 - 16
mag) in the catalog, MisV0850 is probably a new variable star.

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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