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A model-atmosphere analysis of Ap star HD 26385
Authors:Ç Bolcal  D Koçer  T Koktay  T Güzel
Institution:(1) Present address: Physics Department, Faculty of Science, University of Istanbul, Turkey;(2) Present address: Astronomy and Space Science Department, University of Istanbul, Turkey
Abstract:An abundance analysis using photographic region spectrograms and fully line-blanketed model atmospheres has been performed for the chemically peculiar (CP) star HD 26385. Model parameters were determined from Hgamma-profile and photometric data. Its pattern of abundance shows that HD 26385 is typically Ap Si-star.
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