Image Details

Choose export citation format:

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 6.

IV (top panel), KS (middle panel), and FT (bottom panel) significance tests to search for constant period spacings in the set of periods of WD J0049−2525. The vertical thick black dashed lines indicate the possible period spacings present in the star as indicated by the tests (see the main text for details).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse