CAOSP abstracts, Volume: 27, No.: 3, year: 1998
- Author(s): CASTELLI, F.
- Journal: Contributions of the Astronomical Observatory Skalnate Pleso,
vol. 27, no. 3, p. 192-196.
- Date: 04/1998
- Title: The energy distribution of Beta CrB for the specific stellar abundances
- Keyword(s): STARS: CHEMICALLY PECULIAR, STARS: ENERGY DISTRIBUTION
- Pages: 192 -- 196
The comparison of the observed and computed energy distributions
of Beta CrB has shown that a model with the specific chemical
composition of the star can account for the visual energy distribution,
while it is still unable to reproduce ultraviolet observations shortward
of 1700 Angstroms. Furthermore, the predicted absorption of strong Fe II
and Mg II UV lines is much larger than the observed one.
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