Fig. 1.
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Run of general relativistic correction factors ℋ, 𝒢, 𝒱, and ℛ (black, blue, red, and pink lines, respectively) for 1.29, 1.33, 1.35, and 1.369 M⊙ white dwarf models at log L/L⊙ = −3 in terms of the fractional radius. Dashed lines in the bottom right panel illustrate the behavior of the same factors for a 1.369 M⊙ model at log L/L⊙ = −0.4.
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