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Paper: Modeling Formation of Clouds of Heavy Elements in the Magnetic Atmospheres of Hot Stars
Volume: 511, Non-Stable Universe: Energetic Resources, Activity Phenomena and Evolutionary Processes
Page: 216
Authors: Alecian, G.
Abstract: Magnetic A and B main-sequence stars present strange inhomogeneous distributions of metals on their surface. These stars constitute the well-known group of chemically peculiar magnetic stars (ApBp stars). The atmospheres of these stars are known to be strongly affected by atomic diffusion, and a new generation of modeling tools is appearing to take into account the complexity of physical processes in play. In this talk, I will present recent results of 3D numerical modeling of abundance distributions in these atmospheres.
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