NNo       GCVS          J2000.0        Type       Max       Min I        Min II      Epoch(JD24..) Year        Period        M-m/D    Spectrum       References  Other design. 
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780471 |V0471 Tau *|035025.0+171447 |EA/D/RS+X |  9.40   |   9.71     |            |V |45612.38065 |     |     0.52118301     |06   |K0Vea+DA         |10059 05120|
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______________The positional information: ___________________________
  NNo     GCVS            J2000.0         p.m.(as/yr) Epoch     Ident.
----------------------------------------------------------------------
780471 |V0471 Tau |035024.97 +171447.4 |+0.130 -0.023|2000.0  | |Hip
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_______________Cross-identifications:_______________
V0471 Tau     = BD   +16 0516                 |     
V0471 Tau     = G    007-023                  |     
V0471 Tau     = GSC  1252.00212               |     
V0471 Tau     = Hip  017962                   |     
V0471 Tau     = WD   0347+171                 |     
V0471 Tau     = X    03476+171                |     
____________________________________________________

      Reference to a chart or photograph:
05120. H.L.Giclas, R.Burnham, N.G.Thomas, Lowell Publ, N118, 1962.

      Reference to a study of the star:
10059. C.Ibanoglu, S.Evren, IBVS N2573, 1984.
__________________________________________________________________
      Remark:         
    The member of the Hyades cluster. mu alpha =  + 0.117",
    mu delta = -0.020".
    EA/D/(RS + WD) + XP. d = 0.0625P.
    There occurs a total eclipse of the white dwarf in
    Min I (A = 0.04m V, 0.36m U).
    P var. Min I = 2440612.67083 + 0.52118321d*E
    (JD2440570 - 970) [06250]; Min I = 2440898.80038 +
    0.52118376d*E (JD2440880 - 41360), Min I =
    2441665.46153 + 0.52118329d*E (JD2441660 -
    42100) [10058]; since JD2441900 - see Table.
    Wave-like distorsion with the amplitude from 0.05m
    up to 0.27m and with the period close to the orbital
    one is observed in the light curve outside eclipses;
    sometimes there are also flares. The wave is migrating on
    phase in the direction of phase decreasing
    with a migration period of 191d [10060] or ~250d
    [10061]. The period of white dwarf rotation derived
    through X-ray observations Ppuls = 554.73s [10062].

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