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The Structure of Colliding Stellar Winds
Published online by Cambridge University Press: 03 August 2017
Abstract
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We report on progress in the theoretical modelling of colliding winds in WR binary systems, concentrating on two WR+O systems, namely V444 Cygni, and HD 193793.
- Type
- Session IV. Binaries
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- Copyright
- Copyright © Kluwer 1991
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