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Radiation-accellerated ions in hot star winds: heating and “turbulence” effects
Published online by Cambridge University Press: 26 May 2016
Extract
In the papers by Vilkoviskij (1981), Vilkoviskij and Tambovtzeva (1988) and Springmann and Pauldrach (1992) it was shown that ions can reach velocities relative to the wind plasma when the radiation pressure force exceeds the protons frictional force.
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- 7. OB Stellar Winds
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- Copyright © Kluwer 1994