Hostname: page-component-848d4c4894-ndmmz Total loading time: 0 Render date: 2024-05-31T11:58:30.944Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Lucy, L.B.: 1979, Ap. J. 163, 95.CrossRefGoogle Scholar
Lucy, L. B., and Solomon, P.M.: 1970, Ap. J. 159, 879.Google Scholar
McCluskey, G.E. Jr., and Kondo, Y.: 1976, Ap. J. 208, 760.CrossRefGoogle Scholar
McCluskey, G.E. Jr., Kondo, Y., and Morton, D.C.: 1975, Ap. J. 201, 607.CrossRefGoogle Scholar