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An alternative explanation of the EUV spectrum of the white dwarf G191–B2B invoking a stratified H+He envelope including heavier elements
Authors:M A Barstow  & I Hubeny
Institution:Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH,;Laboratory for Astronomy and Solar Physics, NASA/GSFC, Greenbelt, Maryland, MD 20711 USA
Abstract:
Keywords:stars: abundances  stars: atmospheres  stars: individual: G191–B2B  stars: white dwarfs  ultraviolet: stars  X-rays: stars
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