Manifold spirals in barred galaxies with multiple pattern speeds
C. Efthymiopoulos, M. Harsoula, G. Contopoulos

TL;DR
This paper extends manifold theory to include multiple pattern speeds in barred galaxies, showing that complex, time-varying spiral structures can be supported by the dynamics of multiple coexisting modes.
Contribution
It introduces a generalized manifold framework allowing for different pattern speeds, revealing new unstable orbit types and their role in forming recurrent, time-varying spiral structures.
Findings
Manifolds produce time-varying spiral segments and pseudorings.
Structures repeat periodically, supporting recurrent spiral phenomena.
Multiple pattern speeds lead to complex, dynamic galactic morphologies.
Abstract
In the manifold theory of spiral structure in barred galaxies, the usual assumption is that the spirals rotate with the same pattern speed as the bar. Here we generalize the manifold theory under the assumption that the spirals rotate with different pattern speed than the bar. More generally, we consider the case when one or more modes, represented by the potentials V_2, V_3, \ldots, co-exist in the galactic disc in addition to the bar's mode V_{bar}, but rotate with pattern speeds \Omega_2, \Omega_3, \ldots incommensurable between themselves and with \Omega_{bar}. Through a perturbative treatment (assuming that V_2,V_3... are small with respect to V_{bar}) we then show that the unstable Lagrangian points L_1, L_2 of the pure bar model (V_{bar},\Omega_{bar}) are `continued' in the full model as periodic orbits, when we have one extra pattern speed different from \Omega_{bar}, or as…
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