Self-Consistent Diffusion in Low Mass Hot Stars

Details Self-Consistent Diffusion in Low Mass Hot Stars Self-Consistent Diffusion in Low Mass Hot Stars

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..372..213b&link_type=abstract

15th European Workshop on White Dwarfs ASP Conference Series, Vol. 372, proceedings of the conference held 7-11 August, 2006 in

Astronomy and Astrophysics

Astronomy

Scientific paper

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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