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Mass Flow Analysis of the Ultraviolet Spectrum of UW Canis Majoris

Published online by Cambridge University Press:  14 August 2015

H. Drechsel ,
Y. Kondo ,
G.E. McCluskey Jr.  and
J. Rahe
H. Drechsel
Affiliation:
Remeis-Sternwarte Bamberg Astronomical Institute University Erlangen-Nuremberg, F.R.G.
Y. Kondo
Affiliation:
Department of Astronomy University of Pennsylvania Philadelphia, PA, U.S.A.
G.E. McCluskey Jr.
Affiliation:
Department of Mathematics Lehigh University Bethlehem, PA, U.S.A.
J. Rahe
Affiliation:
Laboratory for Astronomy and Solar Physics NASA-Goddard Space Flight Center Greenbelt, MD, U.S.A.

Abstract

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The ultraviolet spectrum of the close binary UW CMa (= HD 57060; 07f Ia + 0-B), obtained with the COPERNICUS (OAO-3) and IUE satellites, is analyzed in terms of a comparison between observed P Cygni resonance line profiles and theoretical calculations in an expanding model atmosphere.

Type
IV. Massive Binary Systems
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 195 - 198
Copyright
Copyright © Reidel 1980 

References

Drechsel, H., Kondo, Y., McCluskey, G.E. Jr., and Rahe, J.: 1979, Astron. Astrophys., in press.Google Scholar
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McCluskey, G.E. Jr., Kondo, Y., and Morton, D.C.: 1975, Ap. J. 201, 607.CrossRefGoogle Scholar