A 3D atmosphere simulation of the cold Jupiter WD 1856+534 b produces temperature, chemistry, wind, and emission-spectrum predictions across six metallicity and internal-heat scenarios.
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Modelling the 3D atmospheric structure of the cold Jupiter WD1856+534b orbiting a white dwarf
A 3D atmosphere simulation of the cold Jupiter WD 1856+534 b produces temperature, chemistry, wind, and emission-spectrum predictions across six metallicity and internal-heat scenarios.