Phase-space distortion as a key to unraveling galactic bar buckling
Viktor D. Zozulia, Natalia Ya. Sotnikova, and Anton A. Smirnov

TL;DR
This paper uses action-angle variables to analyze the resonant structure of galactic bars during buckling, revealing how orbit transformations contribute to the formation of boxy/peanut-shaped bulges and phase space asymmetries.
Contribution
It introduces a novel analysis of the resonant structure of galactic bars during buckling using action-angle variables, highlighting phase space distortions and orbit transformations.
Findings
Resonant orbit transformations lead to bulge formation.
Phase space asymmetries develop during buckling.
Orbital fixed points can disappear, affecting symmetry.
Abstract
For the first time, we investigate the resonant structure of -body galactic bar at the stage of buckling using action-angle variables. We studied the evolution of vertical actions () and angles associated with vertical resonance () for all orbits in the bar. For this purpose, we divide the orbits into types according to the behavior (libration or circulation) of their resonant angle with respect to fixed points and (vertical resonance). We show that during buckling, flat bar orbits circulating with increasing transformed into banana-shaped librating orbits (resonant capture) or circulating orbits with decreasing (resonant heating). The orbital transformation is accompanied by an increase in and the formation of a boxy/peanut-shaped (B/PS) bulge. During…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
