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Properties and Nature of Be Stars. 12. The UV Line Spectrum of KX And - Is There a Hot Primary?

Štefl, S.

Seven high-resolution IUE spectrograms of the Be star KX And were investigated by the standard method of comparison of the observed and theoretical spectra. The whole ultraviolet line spectrum can be described quite well by a model spectrum, corresponding to Kurucz's model with T_eff = 9000 - 10000K and log g = 2.00. A detailed identific…