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Seismic Signatures of the 12C(α, γ)16O Reaction Rate in White Dwarf Models with Overshooting

  • Authors: Morgan T. Chidester, F. X. Timmes, Ebraheem Farag

Morgan T. Chidester et al 2023 The Astrophysical Journal 954 .

  • Provider: AAS Journals

Caption: Figure 6.

Top to bottom: mass fractions of 12C and 16O; B profile; normalized weight function profile for the g6 mode; normalized weight function profile for the g2 mode. The left column shows the NOV results, and the right column shows the OV results. Both figures are for σ = 0.0, T eff = 10,000 K. The R1–R4 region boundaries are indicated by dashed vertical lines. An interactive figure is provided in the online version. Its functionality compares the NOV and OV diagrams, as structured in this figure, for any given σ i 12C(α, γ)16O reaction rate. To use the interactive figure, click on the “sigma” slider at the top, and slide through indices 0 through 12. Sliding through each index provides the user the side-by-side comparison of the diagrams for the respective σ i 12C(α, γ)16O reaction rate used in the evolution. Index 0 starts at σ −3.0 and index 12 ends at σ 3.0.

An interactive version of this figure is available in the online journal.

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