New Takamizawa variable (TmzV900) Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable star (TmzV900). TmzV900 = GSC4058.831 022222.61 +665128.6 (2000.0) 12.88 1 N = GSC4058.831 022222.66 +665128.5 (2000.0) 13.14 1 = USNO1500.02380557 022222.630 +665128.23 (2000.0) 11.8 17.0 = IRAS02183+6637 021819.3 +663745 (1950.0) F12=0.63 F25=0.17 F60=0.40L F100=7.58L VAR=60 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 = 022222.3 +665124 (2000.0) IRAS02183+6637 0.632 0.178 0.400L 7.251L 60% = 022222.3 +665124 (2000.0) SSC02183+6637 0.632 0.178 0.400L 7.251L = 022222.6 +665128 (2000.0) CS336 - - 10.1 - Takamizawa's comment: The star may be a semiregular variable with a range of 12.9-14.0p. Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code TmzV900 19950127.432 131p Tmz.VSOLJ TmzV900 19960922.656 135p Tmz.VSOLJ TmzV900 19970613.737 137p Tmz.VSOLJ TmzV900 19980116.420 140p Tmz.VSOLJ TmzV900 19980629.693 137p Tmz.VSOLJ TmzV900 19991128.440 132p Tmz.VSOLJ TmzV900 20000902.687 129p Tmz.VSOLJ TmzV900 20011023.613 130p 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>