par Behara, Natalie Thérèse ;Jeffery, Simon
Référence Astronomical Society of the Pacific conference series, 372, page (213)
Publication Publié, 2007
Référence Astronomical Society of the Pacific conference series, 372, page (213)
Publication Publié, 2007
Article révisé par les pairs
Résumé : | 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. |