ar X iv : a st ro - p h / 98 05 04 7 v 1 6 M ay 1 99 8 The energy distribution of β CrB for the specific stellar abundances
نویسنده
چکیده
The comparison of the observed and computed energy distributions of β CrB has shown that a model with the specific chemical composition of the star can account for the visual enery distribution, while it is still unable to reproduce ultraviolet observations shortward of 1700Å. Furthermore, the predicted absorption of strong Fe ii and Mg ii UV lines is much larger than the observed one.
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