A 3D hydrodynamic model with self-consistent hydrogen-helium chemistry shows stellar winds compress escaping hot-Jupiter atmospheres and suppress the 1083 nm helium triplet signal, while a young star's strong XUV flux deepens transits 3.3-fold.
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A Self-Consistent 3D Hydrodynamic Model for Helium Transit Signatures in Evaporating Hot Jupiters
A 3D hydrodynamic model with self-consistent hydrogen-helium chemistry shows stellar winds compress escaping hot-Jupiter atmospheres and suppress the 1083 nm helium triplet signal, while a young star's strong XUV flux deepens transits 3.3-fold.