Abstract
We present a FUSE abundance analysis of EC14026 stars. We compare the abundances of heavy elements in the atmospheres of EC14026 stars to non-pulsating stars with similar atmospheric parameters, and investigate whether weak stellar winds could explain the coexistence of variable and non-variable sdB stars in the log g – Teff diagram. We also present preliminary results on time-dependent diffusion calculations of iron in presence of radiative levitation and mass loss, and show how weak stellar winds can affect the diffusive equilibrium between gravitational settling and radiative support.
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Chayer, P., Fontaine, G., Fontaine, M. et al. FUSE Observations of EC14026 Stars. Astrophys Space Sci 291, 359–366 (2004). https://doi.org/10.1023/B:ASTR.0000044344.92680.b8
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DOI: https://doi.org/10.1023/B:ASTR.0000044344.92680.b8