Figure 5 from A NEW GENERATION OF LOS ALAMOS OPACITY TABLES

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A NEW GENERATION OF LOS ALAMOS OPACITY TABLES

Authors: J. Colgan, D. P. Kilcrease, N. H. Magee, M. E. Sherrill, J. Abdallah Jr., P. Hakel, C. J. Fontes, J. A. Guzik, and K. A. Mussack

2016 The Astrophysical Journal 817 116.

Provider: AAS Journals

Caption: Figure 5.

Logarithmic opacity derivative with respect to temperature for ATOMIC and OPAL tables with Z = 0.01, X = 0.80, and log R = −1.5. The larger gradients for the ATOMIC table opacities at the convection-zone base (log T = 6.3) and at ∼0.2–0.3 ﹩{R}_{\odot }﹩ (log T ∼ 6.8) in the solar interior are responsible for the differences in sound-speed gradients between models seen in Figure 4.

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