Modellatmosphärenanalyse von heißen Begleitern Roter Riesen und Überriesen.

Physics

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Scientific paper

The present work presents an investigation on 40 hot companions of red giants and supergiants (program stars) and on 16 comparison stars of spectral type ≡B. The interpretation of ultraviolet flux distributions (as concluded from ≡180, ≡40 high and low resolution IUE-spectra available for program stars, comparison stars, respectively) is performed by means of Kurucz model stellar atmospheres.

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