Figure 4 from The Impact of White Dwarf Luminosity Profiles on Oscillation Frequencies

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The Impact of White Dwarf Luminosity Profiles on Oscillation Frequencies

Authors: F. X. Timmes, Richard H. D. Townsend, Evan B. Bauer, Anne Thoul, C. E. Fields, and William M. Wolf

2018 The Astrophysical Journal Letters 867 L30.

Provider: AAS Journals

Caption: Figure 4.

Weight functions for four adiabatic modes of the original and relaxed models; a pair of adjacent radial order ℓ = 1 modes (top row) and a pair of adjacent radial order ℓ = 2 modes (middle row). The original and relaxed models share the same mass fraction profile (bottom row).

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