New Takamizawa variable (TmzV922) Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable star (TmzV922). TmzV922 = GSC4297.598 012918.00 +680009.0 (2000.0) 10.94 1 = GSC4297.598 012918.07 +680008.7 (2000.0) 11.03 1 = USNO1575.00932948 012918.040 +680008.78 (2000.0) 11.5 14.4 * = IRAS01257+6744 012542.6 +674437 (1950.0) F12=0.91 F25=0.25 F60=0.40L F100=2.29L VAR= 0 LRS=-1 possibly I: oxygen-rich non-variable star without circumstellar shell or VIa: non-variable star with relatively cold dust at large distance, may be carbon-rich = 012917.4 +680006 (2000.0) IRAS01257+6744 0.892 0.253 0.400L 2.297L 0% = 012917.4 +680006 (2000.0) SSC01257+6744 0.892 0.253 0.400L 2.297L Takamizawa's comment: The star may be a semiregular variable with a range of 11.1-11.8p. Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code TmzV922 19950127.432 118p Tmz.VSOLJ TmzV922 19960922.656 116p Tmz.VSOLJ TmzV922 19970613.737 114p Tmz.VSOLJ TmzV922 19980116.420 117p Tmz.VSOLJ TmzV922 19980629.693 118p Tmz.VSOLJ TmzV922 19991128.440 117p Tmz.VSOLJ TmzV922 20000902.687 115p Tmz.VSOLJ TmzV922 20011023.613 111p Tmz.VSOLJ Observer's code: Tmz: K.Takamizawa (Saku-machi,Nagano,Japan) SASS (Saku All Sky Survey) Inst.: 10cmR F4 twin patrol cameras and 25cm F2.8 Baker-Schmidt camera T-Max400 120 Comparison stars mag.:GSC Relayed from Kesao Takamizawa <k-takamizawa@nifty.ne.jp>