Multicomponent stellar winds and chemical peculiarity in A stars

Computer Science

Scientific paper

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Hydrodynamics, Stars: Mass Loss, Stars: Early-Type, Stars: Winds.

Scientific paper

We calculate multicomponent radiatively driven stellar wind models
suitable for A stars. We discuss the possible decoupling of individual
elements from the stellar wind and its influence on the chemical
peculiarity of these stars. We obtain a range of stellar parameters for
different types of multicomponent flow.

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