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CP#AP WORKSHOP
10. - 14. September 2007
Vienna, Austria
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The classical chemically peculiar stars of the upper main sequence
provide excellent test objects for astrophysical processes
like diffusion, convection, and stratification in stellar
atmospheres in the (non-)presence of rather strong magnetic fields.
These mechanisms for stars, both in the Milky Way and its surrounding
stellar systems, contribute important knowledge to stellar evolution
under different local circumstances.
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