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Cited article:

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Solar Models and Astrophysical S-factors Constrained by Helioseismic Results and Updated Neutrino Fluxes

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The Astrophysical Journal 970 (1) 38 (2024)
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Grids of rotating stellar models with masses between 1.0 and 3.0M⊙

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THE EFFECTS OF ROTATION ON THE MAIN-SEQUENCE TURNOFF OF INTERMEDIATE-AGE MASSIVE STAR CLUSTERS

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Open issues in probing interiors of solar-like oscillating main sequence stars 1. From the Sun to nearly suns

M J Goupil, Y Lebreton, J P Marques, R Samadi and F Baudin
Journal of Physics: Conference Series 271 012031 (2011)
https://doi.org/10.1088/1742-6596/271/1/012031

SEISMIC AND DYNAMICAL SOLAR MODELS. I. THE IMPACT OF THE SOLAR ROTATION HISTORY ON NEUTRINOS AND SEISMIC INDICATORS

S. Turck-Chièze, A. Palacios, J. P. Marques and P. A. P. Nghiem
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Eddy viscosity and turbulent Schmidt number by kink-type instabilities of toroidal magnetic fields

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Solar Models with Revised Abundances and Opacities

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