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Mass Transfer and Line Profiles - WZ Sge

Published online by Cambridge University Press:  12 April 2016

Z. Šima
Affiliation:
Astronomical Institute of ČSAV, Praha, Czechoslovakia
P. Hadrava
Affiliation:
Astronomical Institute of ČSAV, Praha, Czechoslovakia

Abstract

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The calculation of a gas stream offers two modes of the stream. In any case the stream cannot be detected optically. The calculated line profiles caused by the disc are demonstrated.

Type
II. Radio, IR and Optical Observations
Copyright
Copyright © Reidel 1987

References

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