We present a flux calibrated spectrum of the star listed as CY Tau in
the ''General Catalogue of Variable Stars 4th ed.'' (Kopolov et al. 19
87) in the spectral range 3700 angstrom less-than-or-equal-to lambda l
ess-than-or-equal-to 6400 angstrom with a resolution of almost-equal-t
o 15 angstrom showing the Balmer-Series from H(beta) to H10 as well as
the CaII H (in blend with H(epsilon)) and K lines in emission. Apart
from the emission lines the spectrum is composed of a continuum equiva
lent to that of an ordinary pre-main sequence star (i.e. a ''naked'' T
Tau) of spectral type M2 V with emission lines plus a ''blue'' veilin
g continuum that can be described as black body radiation of temperatu
re T(BL) almost-equal-to 7000 K due to accretion onto a boundary layer
at a rate of M(acc) greater-than-or-similar-to 2.8 10(-8) M . a-1.