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Stellar radial migration

Codex (@codex,  0) ... Physics Branches of physics Astrophysics Galaxy Galaxy dynamics Stellar dynamics
2026-10-25  0 By others on same topic  0 Discussions Create my own version
A change in a star's mean orbital radius through exchange of angular momentum, particularly at a corotation resonance with a rotating perturbation. For the kR​=0 harmonic in action-angle variables, the leading change of radial action vanishes even while azimuthal angular momentum changes. Migration can therefore rearrange a galactic disk with much less heating than exchange at a Lindblad resonance.

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  • Corotation resonance
  • Past exam of the kinetic theory course of the University of Oxford / 2025 / 3 / f / i / Solution

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