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Asteroseismology of WD J004917.14−252556.81, the Most Massive Pulsating White Dwarf

Authors: Ozcan Caliskan, Murat Uzundag, Mukremin Kilic, Francisco C. De Gerónimo, Adam Moss, Alejandro H. Córsico, Steven G. Parsons, Ingrid Pelisoli, Gracyn Jewett, Alberto Rebassa-Mansergas, Alex J. Brown, Vikram S. Dhillon, Pierre Bergeron

Ozcan Caliskan et al 2025 The Astrophysical Journal 988 .

Provider: AAS Journals

Caption: Figure 1.

Model fits (red lines) to the normalized Balmer line profiles (black lines) of WD J0049−2525. The 3D hydrodynamical corrections are included in the best-fitting model parameters.

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