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The unusual A-star VW Ari: chemical composition revisited

I. V. Chernyshova·S. M. Andrievsky·V. V. Kovtyukh·D. E. Mkrtichian
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Abstract

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.

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I. V. Chernyshova, S. M. Andrievsky, V. V. Kovtyukh, D. E. Mkrtichian. 1998-05-14. The unusual A-star VW Ari: chemical composition revisited. https://arxiv.org/abs/astro-ph/9805185

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