M.R. Burleigh, M.A. Barstow and P.D. Dobbie
We have analysed the EUVE spectrum of the DAO white dwarf RE J0720-318. In contrast to the optical spectrum, which can only be fitted with a homogeneously mixed H+He atmosphere, we find the EUVE spectrum can only be matched with a stratified structure. The H layer mass of 3E-14 solar masses is a factor of ~10 below upper limits from previous EUVE observations of white dwarfs. In addition, we detect an unprecedented HeI/H ratio of ~1 for the absorbing column along the line of sight, implying an H ionization fraction >90% if all this material resides in the local ISM. We suggest that, since this is a close pre-CV binary system, most of the helium probably lies within the immediate vicinity of the star, possibly in the form of a circumbinary disk left over from the common envelope (CE) phase. These results have important implications for our understanding of the evolutionary status of DAO white dwarfs in particular, and for post-CE binaries in general.
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