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Fig. 8.

image

Internal chemical structure (upper panel) and squared Brunt–Vaïsälä and Lamb frequencies for ℓ = 1 and ℓ = 2 (lower panel) corresponding to our best-fit ultra-massive DA WD model for BPM 37093 with a stellar mass M* = 1.16 M, an effective temperature Teff = 11 653 K, a H envelope mass of log(MH/M*)∼ − 6, and a crystallised mass fraction of Mcr = 0.92M.

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