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Title: On the Impact of 22 Ne on the Pulsation Periods of Carbon–Oxygen White Dwarfs with Helium-dominated Atmospheres

We explore changes in the adiabatic low-order g-mode pulsation periods of 0.526, 0.560, and 0.729Mcarbon–oxygen white dwarf models with helium-dominated envelopes due to the presence, absence, and enhancement of22Ne in the interior. The observed g-mode pulsation periods of such white dwarfs are typically given to 6−7 significant figures of precision. Usually white dwarf models without22Ne are fit to the observed periods and other properties. The rms residuals to the ≃150−400 s low-order g-mode periods are typically in the range ofσrms≲ 0.3 s, for a fit precision ofσrms/P≲ 0.3%. We find average relative period shifts of ΔP/P≃ ±0.5% for the low-order dipole and quadrupole g-mode pulsations within the observed effective temperature window, with the range of ΔP/Pdepending on the specific g-mode, abundance of22Ne, effective temperature, and the mass of the white dwarf model. This finding suggests a systematic offset may be present in the fitting process of specific white dwarfs when22Ne is absent. As part of the fitting processes involves adjusting the composition profiles of a white dwarf model, our study on the impact of22Ne can provide new inferences on the derived interior mass fraction profiles. We encourage routinely including22Ne mass fraction profiles, informed by stellar evolution models, to future more » generations of white dwarf model-fitting processes.

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Award ID(s):
1663696 1707419 1927130
Publication Date:
Journal Name:
The Astrophysical Journal
Page Range or eLocation-ID:
Article No. 24
DOI PREFIX: 10.3847
Sponsoring Org:
National Science Foundation
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