ASTROPHYSICS AND SPACE SCIENCE, sa.2, ss.237-247, 1991 (SCI-Expanded)
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 H-gamma-profile and photometric data. Its pattern of abundance shows that HD 26385 is typically Ap Si-star.