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Mass Flow Analysis of the Ultraviolet Spectrum of UW Canis Majoris
Published online by Cambridge University Press: 14 August 2015
Abstract
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
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- Copyright © Reidel 1980