Fig. 3.
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Rest mass m (upper panel) and density of rest mass (bottom panel) for the general relativity and Newtonian cases (red solid and black dashed lines, respectively) in terms of radial coordinate for 1.369 M⊙ white dwarf models at advanced stage of evolution. Dotted lines in the bottom panel depict the situation for the 1.35 M⊙ models.
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