Dear colleagues, New variable star discovery by the MISAO Project (MisV0913). MisV0913 R.A. 17h56m34s.93 Decl. -19o51'00".3 (2000.0) Mag. 11.9C-13.2C Type ? = USNO-A2.0_0675.23493693 17 56 34.932 -19 51 00.27 12.2R 18.2B = IRAS 17536-1950 R.A.=17 56 34.74 Decl.=-19 51 02.4 (19 x 5", p.a.=90) flux(12)=7.01 flux(25)=3.89 flux(60)=<1.66 flux(100)=<20.76 78% variable http://vsnet.aerith.net/misao/data/MisV/MisV0913.gif MisV0913 20000211.83264 119C Mis image="KenIchi Kadota" MisV0913 20000211.83576 119C Mis image="KenIchi Kadota" MisV0913 20000216.83476 128C Mis image="KenIchi Kadota" MisV0913 20000216.83558 128C Mis image="KenIchi Kadota" MisV0913 20000216.83634 129C Mis image="KenIchi Kadota" MisV0913 20000216.83791 127C Mis image="KenIchi Kadota" MisV0913 20000216.83966 128C Mis image="KenIchi Kadota" MisV0913 20000224.81625 129C Mis image="KenIchi Kadota" MisV0913 20000224.81719 129C Mis image="KenIchi Kadota" MisV0913 20000224.81855 128C Mis image="KenIchi Kadota" MisV0913 20000308.82081 128C Mis image="KenIchi Kadota" MisV0913 20000308.82168 128C Mis image="KenIchi Kadota" MisV0913 20000319.79674 132C Mis image="KenIchi Kadota" MisV0913 20000319.79822 131C Mis image="KenIchi Kadota" MisV0913 20000319.79890 130C Mis image="KenIchi Kadota" Seiichi Yoshida, MISAO Project; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0913. It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Kadota, then confirmed by Yoshida. 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/