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      Tidal Flows in asynchronous binaries: The beta-factor

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          Abstract

          We discuss the potential role that tidal flows in asynchronous binary stars may play in transporting chemically enriched material from deep layers towards the surface and the corresponding observational consequences of these processes. We suggest that the time-dependent velocity field induced by asynchronous rotation may contribute significantly to the mixing, thus providing a channel for the formation of chemically enriched slowly rotating massive stars.

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          Author and article information

          Journal
          04 December 2013
          Article
          10.1051/eas/1364047
          1312.1372
          25d24d13-f6cd-4f08-8d37-55a559800a89

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          in Setting New Standards in Binary Star Research, A. Tkachenko & K. Pavlovski (eds), EAS Publication Series, in Press
          astro-ph.SR

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