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Paper: Self-Consistent Diffusion in Low Mass Hot Stars
Volume: 372, 15th European Workshop on White Dwarfs
Page: 213
Authors: Behara, N.T.; Jeffery, C.S.
Abstract: The effects of diffusion in the atmospheres of low mass hot stars have been investigated using a model atmosphere code which includes diffusion self-consistently. The atmospheric structures associated with non-uniform composition are compared to models with homogeneous abundances. We compare preliminary results obtained using these models to observed abundances of chemically peculiar subdwarf B stars.
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