The sign of the disk's radial temperature gradient decides which Lagrange point, L4 or L5, collects more gas around an embedded planet, breaking the classical symmetry of the restricted three-body problem.
, de Gregorio-Monsalvo, I
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Origin of the asymmetric gas distribution near the co-orbital Lagrange points of an embedded planet
The sign of the disk's radial temperature gradient decides which Lagrange point, L4 or L5, collects more gas around an embedded planet, breaking the classical symmetry of the restricted three-body problem.