Dear colleagues, New variable star discovery by the MISAO Project (MisV0830). MisV0830 R.A. 17h57m07s.48 Decl. -32o39'48".2 (2000.0) Mag. 10.3C-11.3C Type ? = USNO-A2.0_0525.30818785 17 57 07.660 -32 39 50.91 13.3R 16.3B = IRAS 17538-3239 R.A.=17 57 06.45 Decl.=-32 39 46.8 (26 x 4", p.a.=92) flux(12)=6.60 flux(25)=3.48 flux(60)=1.25 flux(100)=<69.22 10% variable http://vsnet.aerith.net/misao/data/MisV/MisV0830.gif MisV0830 19990520.68679 113C Mis MisV0830 19990520.68723 112C Mis MisV0830 20000224.84394 103C Mis MisV0830 20000224.84450 103C 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. 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/