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[vsnet-newvar 583] New variable star MisV1009



Dear colleagues,

New variable star discovery by the MISAO Project (MisV1009).

MisV1009
  R.A.  17h54m00s.82
  Decl. -17o52'43".8  (2000.0)
  Mag.  12.8C-13.8C
  Type  SR:
= USNO-A2.0_0675.23250810  17 54 00.817  -17 52 43.78  13.5R  17.6B
= IRAS 17510-1752  R.A.=17 54 00.16  Decl.=-17 52 38.6  (31 x 6", p.a.=82)  flux(12)=1.52  flux(25)=0.84  flux(60)=<0.83  flux(100)=<12.71  34% variable

  http://vsnet.aerith.net/misao/data/MisV/MisV1009.gif

MisV1009 19990212.83565 138C Mis image="KenIchi Kadota"
MisV1009 19990212.83852 137C Mis image="KenIchi Kadota"
MisV1009 19990220.83337 134C Mis image="KenIchi Kadota"
MisV1009 19990220.83426 133C Mis image="KenIchi Kadota"
MisV1009 19990331.75648 129C Mis image="KenIchi Kadota"
MisV1009 19990331.76264 129C Mis image="KenIchi Kadota"
MisV1009 19990331.76437 130C Mis image="KenIchi Kadota"
MisV1009 19990331.78179 139CIR Mis image="KenIchi Kadota"
MisV1009 19990331.78299 139CIR Mis image="KenIchi Kadota"
MisV1009 19990331.78541 139CIR Mis image="KenIchi Kadota"
MisV1009 19990331.79027 128R Mis image="KenIchi Kadota"
MisV1009 19990331.79293 128R Mis image="KenIchi Kadota"
MisV1009 19990331.79547 128R Mis image="KenIchi Kadota"
MisV1009 19990408.76785 136C Mis image="KenIchi Kadota"
MisV1009 19990408.76929 132C Mis image="KenIchi Kadota"
MisV1009 19990413.68201 128C Mis image="KenIchi Kadota"
MisV1009 19990413.68737 128C Mis image="KenIchi Kadota"
MisV1009 19990429.68597 129C Mis image="KenIchi Kadota"
MisV1009 19990429.68708 130C Mis image="KenIchi Kadota"
MisV1009 19990604.61503 133C Mis image="KenIchi Kadota"
MisV1009 19990604.61567 134C Mis image="KenIchi Kadota"
MisV1009 19990604.61653 132C Mis image="KenIchi Kadota"

Seiichi Yoshida, MISAO Project; and KenIchi Kadota, Ageo, Saitama,
Japan, discovered a new variable star MisV1009.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from 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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