Far-ultraviolet colors of B stars with and without emission lines

Details Far-ultraviolet colors of B stars with and without emission lines Far-ultraviolet colors of B stars with and without emission lines

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.

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