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Some Results of the Spectroscopic Study of Four Close Binary Systems of Early Spectral Types

Published online by Cambridge University Press:  25 July 2018

T. S. Galkina*
Affiliation:
Crimean Astrophysical Observatory, Nauchny, Crimea, U.S.S.R.

Extract

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It is necessary to have quantitative estimates of the intensity of lines (both absorption and emission) to obtain the physical parameters of the atmosphere of components.

Some years ago at the Crimean observatory we began the spectroscopic investigation of close binary systems of the early spectral type with components WR, Of, O, B to try and obtain more quantitative information from the study of the spectra of the components.

Type
Third Session
Copyright
Copyright © 1971

References

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