Figure 3 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 3.

Differences between the adiabatic frequencies ν of ℓ = 1 and ℓ = 2 g-modes in the relaxed and original MESA models. Selected modes are labeled by their radial order ﹩\tilde{n}﹩. The shaded region marks the range of frequencies seen in the Kepler observations of KIC 08626021.

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