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The circumstellar matter in the Be + K binary KX and seen in the uv spectra *

Published online by Cambridge University Press:  04 August 2017

S. Štefl
S. Štefl*
Affiliation:
Astronomical Institute 251 65 Ondřejov, Czechoslovakia

Extract

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KX And (HD 218393) belongs to well-known and often observed Be stars. The periodicity of spectroscopic characteristics as well as other observations led to the conclusion that the star is a peculiar interacting binary (Harmanec et al. 1980). The aim of this paper is to present the phase-dependent behaviour of the UV spectrum of the star.

Type
Symbiotic Stars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 493 - 495
Copyright
Copyright © Reidel 1987 

References

Harmanec, P., Horn, J., Koubský, P., Žďárský, F., Kříž, S., Pavlovski, K.: 1980, Bull. Astron. Int. Czechosl. 31, 144.Google Scholar
Hubený, I. Štefl, S. Harmanec, P.: 1985, Bull. Astron. Inst. Czechosl. 34, 214.Google Scholar
Kurucz, R. L.: 1979, Astrophys. J. Suppl. Ser. 40, 1.Google Scholar