Dear colleagues, New variable star discovery by the MISAO Project (MisV0917). MisV0917 R.A. 19h01m23s.15 Decl. +10o47'33".7 (2000.0) Mag. 12.6C-13.5C Type SR? = USNO-A2.0_0975.13892128 19 01 23.149 +10 47 33.72 14.8R 17.5B = IRAS 18590+1043 R.A.=19 01 22.47 Decl.=+10 47 30.2 (45 x 8", p.a.=79) flux(12)=1.10 flux(25)=0.49 flux(60)=<0.73 flux(100)=<7.99 21% variable http://vsnet.aerith.net/misao/data/MisV/MisV0917.gif MisV0917 19990429.71549 133C Mis image="KenIchi Kadota" MisV0917 19990429.71593 133C Mis image="KenIchi Kadota" MisV0917 19990707.65926 130C Mis image="KenIchi Kadota" MisV0917 19990707.65968 129C Mis image="KenIchi Kadota" MisV0917 19990923.48074 134C Mis image="KenIchi Kadota" MisV0917 19990923.48150 135C Mis image="KenIchi Kadota" MisV0917 20000505.63022 126C Mis image="Nobuo Ohkura" MisV0917 20000505.63207 126C Mis image="Nobuo Ohkura" Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0917. It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ohkura comparing with 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/