4.7 Article

Resonant capture, counter-rotating discs, and polar rings

Journal

Publisher

OXFORD UNIV PRESS
DOI: 10.1046/j.1365-8711.2000.03653.x

Keywords

galaxies : formation; galaxies : general; galaxies : kinematics and dynamics

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We suggest that polar rings and/or counter-rotating discs in flattened galaxies can be formed from stars captured at the Binney resonance, where the rate of precession of the angular momentum vector of a disc star equals the pattern speed of a triaxial halo. If the halo pattern speed is initially retrograde and slowly decays to zero, stars can be trapped as the Binney resonance sweeps past them, and levitated into polar orbits. If the halo pattern speed is initially retrograde and slowly changes to prograde, trapped stars can evolve from prograde to retrograde disc orbits.

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