New Takamizawa variable (TmzV876) Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable star (TmzV876). The variable is identified with an A2V-type emission line object with a strong infrared excess. The nature of the object needs to be studied in more detail. TmzV876 = GSC4037.2277 021448.47 +622622.2 (2000.0) 13.05 1 = USNO1500.02271910 021448.478 +622622.17 (2000.0) 12.8 13.9 = IRAS02110+6212 021104.4 +621220 (1950.0) F12=3.02 F25=2.09 F60=3.63L F100=43.64L VAR= 7 LRS=-1 possibly IIIa: variable star with more evolved O-rich c.s. shell or VIb: variable star with relatively hot dust close to the star and relatively cold dust at large distance may be O-rich or VII: variable star with more evolved C-rich circumstellar shell = 021448.4 +622621 (2000.0) HBH10-1 em V=12.9 A2V = 021447.8 +622618 (2000.0) IRAS02110+6212 2.946 2.139 3.780L 44.670L 7% = 021447.8 +622618 (2000.0) SSC02110+6212 2.946 2.139 3.780L 44.670L = 021448.0 +622622 (2000.0) MSX5C_G132.4082+01.1117 -33 -17 2 3 2 -5 V(%):-:-:1:2:4:- Takamizawa's comment: The star may be a semiregular variable with a range of 12.5-13.1p. [See, however, the earlier note. The star seems to be an early type variable star in a dusty environment -- T. Kato] Photographic magnitude estimates by VSOLJ members object YYYYMMDD(UT) mag code TmzV876 19950127.432 125p Tmz.VSOLJ TmzV876 19960922.656 131p Tmz.VSOLJ TmzV876 19971218.478 128p Tmz.VSOLJ TmzV876 19980116.420 127p Tmz.VSOLJ TmzV876 19991128.440 127p Tmz.VSOLJ TmzV876 20000902.678 130p Tmz.VSOLJ TmzV876 20011023.605 131p 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>