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Rotational Velocity Versus Mass Loss in be Stars
Published online by Cambridge University Press: 14 August 2015
Abstract
C IV and Si IV resonance line profiles of 21 Be, B-shell and normal stars are studied with the aim of detecting evidences for mass loss. We found that almost all our sampled stars are loosing mass. A relation between an estimated lower limit for the rate of mass loss and the observed rotational velocity was searched but not found.
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- V. Rotation and Binarity
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- Copyright © Reidel 1982
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