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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 4.

Top two: NOV set’s signature adiabatic pulsation modes shown at T eff = 11,500 K (bright green), and T eff = 10,000 K (blue), respectively. The first panel shows the signal from the g 2 mode; the second shows the signal from the g 6 trapped mode. Bottom: the kinetic energy diagrams for all σ i at T eff = 11,500 K (left) and T eff = 10,000 K (right), respectively. The green dots/lines represent E kin for σ i > 0, gray for σ i < 0, black for σ = 0. The shading of color gets fainter the further away from σ = 0.

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