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The mass of helium in white dwarf stars and the formation and evolution of hydrogen-deficient post-AGB stars
Authors:T M Lawlor  J MacDonald
Institution:Penn State University –Wilkes-Barre Campus, Department of Physics, Lehman, PA 18627, USA;University of Delaware, Department of Physics and Astronomy, Newark, DE 19716, USA
Abstract:
Keywords:stars: AGB and post-AGB  stars: evolution  white dwarfs
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