A model-atmosphere analysis of AP star HD 26385

Details A model-atmosphere analysis of AP star HD 26385 A model-atmosphere analysis of AP star HD 26385

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185..237b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 2, Nov. 1991, p. 237-247. Research supported by Scientific and Te

Astronomy and Astrophysics

Astrophysics

1

A Stars, Abundance, Atmospheric Models, Peculiar Stars, Stellar Atmospheres, Astronomical Photometry, H Gamma Line, Spectrograms

Scientific paper

An abundance analysis using photographic region spectrograms and fully
line-blanketed model atmospheres has been performed for the chemically
peculiar star HD 26385. Model parameters were determined from
H-gamma-profile and photometric data. Its pattern of abundance shows
that HG 26385 is a typical Ap Si-star.

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