New Takamizawa variable (TmzV123) Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable star (TmzV123). TmzV123 = GSC4084.1302 051046.16 +621402.7 (2000.0) 13.45 1 = USNO1500.04123524 051046.166 +621402.57 (2000.0) 11.8 15.1 = IRAS05061+6210 050609.6 +621020 (1950.0) F12=1.44 F25=0.69 F60=0.40L F100=1.20L VAR=19 LRS=-1 possibly II: variable star with 'young' O-rich circumstellar shell or VII: variable star with more evolved C-rich circumstellar shell or VIa: non-variable star with relatively cold dust at large distance, may be carbon-rich = 051044.8 +621400 (2000.0) FSC05061+6210 1.408 0.725 0.149L 1.651L = 051046.8 +621403 (2000.0) IRAS05061+6210 1.430 0.672 0.400L 1.203L 19% = 051046.8 +621403 (2000.0) SSC05061+6210 1.430 0.672 0.400L 1.203L Takamizawa's comment: The star may be a semiregular variable (SR) with a range of 13.4-14.1p. Photographic magnitude estimates by VSOLJ members object YYMMDD(UT) mag code TmzV123 941108.587 136p Tmz.VSOLJ TmzV123 941224.470 134p Tmz.VSOLJ TmzV123 950127.514 140p Tmz.VSOLJ TmzV123 951128.592 141p Tmz.VSOLJ TmzV123 971123.579 140p Tmz.VSOLJ TmzV123 971231.580 135p Tmz.VSOLJ TmzV123 980318.457 137p Tmz.VSOLJ TmzV123 980820.715 137p Tmz.VSOLJ TmzV123 981218.581 141p Tmz.VSOLJ Observer's code: Tmz: K.Takamizawa (Saku-machi,Nagano,Japan) Inst.: 10cmR F4 twin patrol cameras T-Max400 120 Comparison stars mag.:GSC Relayed from Kesao Takamizawa <GHA07243@nifty.ne.jp>