Also independently discovered by Mike Collins in England. Fair is fair. On Mon, 29 Mar 1999 12:44:34 +0900 (JST), you wrote: >> I'm sure the discoverer will chime in here, but SIMBAD shows that this >> star is a mid-M star, so presumably a Mira, located in the background of the >> Hyades cluster. DHK 42 = V1100 Tau = IRAS 04184+2008 = StM 33. > > Other identifications: > >GSC1272.567 042125.33 +201559.4 (2000.0) 14.30 1 >GSC1272.567 042125.45 +201558.6 (2000.0) 14.44 1 >USNO1050.01252584 042125.409 +201558.95 (2000.0) 10.0 13.6 >042125.1 +201559 (2000.0) LMS33 M6 >13.5 >042125.3 +201558 (2000.0) Q1993/009 10.9 <12.0 >042125.6 +201559 (2000.0) IRAS04184+2008 16.000 5.225 0.950 1.696L 99% >042125.6 +201559 (2000.0) SSC04184+2008 16.000 5.225 0.950 1.696L >042126.0 +201559 (2000.0) FSC04185+2008 12.370 4.840 0.923 4.467L >042125.3 +201558 (2000.0) TAUV1100 M 12.5 (15.5 P - - - - >042125.9 +201703 (2000.0) WSV15 > > The last entry (WSV15) shows that this variable was independently discovered >by M. Wakuda. > >Regards, >Taichi Kato