New Takamizawa variable (TmzV742) Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable star (TmzV742). TmzV742 = GSC524.1806 205025.09 +060538.1 (2000.0) 10.10 6 N = GSC524.1806 205025.11 +060537.6 (2000.0) 10.37 1 N = USNO0900.19235440 205025.110 +060537.69 (2000.0) 9.0 12.1 = IRAS20479+0554 204756.7 +055422 (1950.0) F12=39.80 F25=22.90 F60=3.02 F100=1.90 VAR=16 LRS=23 blue, 10micron (silicate) emission, strength=3 IIIa: variable star with more evolved O-rich c.s. shell = 205024.4 +060538 (2000.0) TMSS+10479 = 205024.6 +060537 (2000.0) RAFGL2662 = 205024.7 +060539 (2000.0) EIC840 = 205025.1 +060536 (2000.0) IRAS20479+0554 39.300 23.470 3.155 1.952 16% 2(LRS) = 205025.1 +060536 (2000.0) SSC20479+0554 39.300 23.470 3.155 1.952 = 205025.4 +060541 (2000.0) FSC20479+0554 39.210 23.330 3.583 1.958 = 205025.0 +060538 (2000.0) 1069E 1.92 TYC524.1806.1 plx=-14.2(79.4) (0.09 0.71) = 205025.0 +060537 (2000.0) 1071 1.70 TYC2-524.1806.1 (10.88 0.07) (12.88 0.26) = 205026.9 +060421 (2000.0) DO7021 Takamizawa's comment: The star may be a semiregular variable with a range of 10.0-11.0p. object YYYYMMDD(UT) mag code TmzV742 19940414.731 104p Tmz.VSOLJ TmzV742 19940803.573 107p Tmz.VSOLJ TmzV742 19940810.668 110p Tmz.VSOLJ TmzV742 19940930.524 110p Tmz.VSOLJ TmzV742 19941102.861 109p Tmz.VSOLJ TmzV742 19941127.412 108p Tmz.VSOLJ TmzV742 19941220.385 108p Tmz.VSOLJ TmzV742 19950306.828 108p Tmz.VSOLJ TmzV742 19950401.788 107p Tmz.VSOLJ TmzV742 19950723.647 107p Tmz.VSOLJ TmzV742 19951014.506 102p Tmz.VSOLJ TmzV742 19960318.799 103p Tmz.VSOLJ TmzV742 19960716.701 100p Tmz.VSOLJ TmzV742 19961030.464 103p Tmz.VSOLJ TmzV742 19970309.826 103p Tmz.VSOLJ TmzV742 19970901.582 109p Tmz.VSOLJ TmzV742 19971025.533 107p Tmz.VSOLJ TmzV742 19980402.785 109p Tmz.VSOLJ TmzV742 19990708.626 110p Tmz.VSOLJ TmzV742 20000314.817 109p 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>