| |
 |
| 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. |
|
|
|
|
|
