Distribution functions for resonantly trapped orbits in the Galactic disc

The present-day response of a Galactic disc stellar population to a non-axisymmetric perturbation of the potential has previously been computed through perturbation theory within the phase-space coordinates of the unperturbed axisymmetric system. Such an Eulerian linearized treatment, however, leads...

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Sonraí bibleagrafaíochta
Príomhchruthaitheoirí: Monari, G, Famaey, B, Fouvry, J, Binney, J
Formáid: Journal article
Foilsithe / Cruthaithe: Oxford University Press 2017