Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982iaus...98..419z&link_type=abstract
In: Be stars; Proceedings of the Symposium, Munich, West Germany, April 6-10, 1981. (A83-10301 01-90) Dordrecht, D. Reidel Publi
Astronomy and Astrophysics
Astronomy
B Stars, Emission Spectra, Interstellar Extinction, Spectral Energy Distribution, Stellar Color, Ultraviolet Astronomy, Data Correlation, Far Ultraviolet Radiation, Line Spectra, Shell Stars, Stellar Envelopes, Stellar Spectra
Scientific paper
A method free of interstellar reddening of comparing the energy distributions in the far-UV of Be/shell stars to those of normal B stars is presented. The deviations of Be/shell stars from the sequences of normal stars are correlated with other physical parameters observed in these stars. The largest UV color differences to the sequences of normal stars are found for those Be/shell stars having the largest IR color excesses.
Briot Danielle
Divan Lucienne
Zorec Jean
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