  Seven high-resolution and high S/N CCD spectra were used to derive elemental
abundances in the atmosphere of VW Ari A (T_eff=7200, log g=3.7) which is the
primary component of a visual binary system. The synthetic spectrum technique
applied in the analysis allowed to reveal the following feature: the atmosphere
of this star is strongly deficient in some metals, while light elements have
solar-like abundances. Taking into account these results, one can suggest that
VW Ari A is a lambda Boo-type star. Another argument supporting this
supposition is the following: on the diagrams (b-y)-c_1, (b-y)-m_1 and
(b-y)-beta (Paunzen et al. 1997), VW Ari A falls exactly in the region occupied
by the lambda Boo stars.
  Note also, that a previous analysis (Andrievsky et al. 1995) has shown that
the secondary component of VW Ari has a normal metallicity. Differences in
chemical compositions of the two components appear to be due to the specific
evolution of the primary VW Ari A.
