Dear colleagues, New variable star discovery by the MISAO Project (MisV1088). MisV1088 R.A. 21h16m45s.96 Decl. +46o47'06".7 (2000.0) Mag. 11.2-12.0C Type SR: = GSC 3589-01057 21h16m45s.91 +46o47'07".1 Error:0.2" Mag:13.14 MagError:0.40 Band:1 Class:3 Plate:02RW Flag:F Epoch:14 JUN 1983 = USNO-A2.0 1350.13776306 21h16m45s.974 +46o47'07".32 Mag(R):12.9 Mag(B):17.3 = IRAS 21149+4634 21h16m44s.9 +46o46'54" Ellipse:30x3" P.A.:52 Flux(12):13.85 Flux(25):9.418 Flux(60):1.812 Flux(100):<13.74 Var:0% = 2MASS 211645.978 +464706.99 (2000.0) 6.553 0.000 0.000 http://vsnet.aerith.net/misao/data/MisV/MisV1088.gif MisV1088 20000804.55922 11.29C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20000804.56107 11.19C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20000804.56292 11.19C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20000917.48665 11.59C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20000917.48850 11.62C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20000917.49035 11.68C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20001009.45928 11.94C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20001009.46112 11.93C Mis KAF-1600 - Nobuo_Ohkura MisV1088 20001009.46297 12.02C Mis KAF-1600 - Nobuo_Ohkura Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and KenIchi Kadota, MISAO Project, discovered a new variable star MisV1088. It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura, and confirmed by KenIchi Kadota. The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), and Seiichi Yoshida. The magnitude are measured automatically by the PIXY system 2. About the MISAO Project and the PIXY system 2: http://vsnet.aerith.net/misao/ -- Seiichi Yoshida comet@aerith.net http://vsnet.aerith.net/