Trimodal structure of Hercules stream explained by originating from bar resonances
Tetsuro Asano, Michiko S. Fujii, Junichi Baba, Jeroen B\'edorf, Elena, Sellentin, Simon Portegies Zwart

TL;DR
This study uses a detailed N-body simulation of the Milky Way to explain the trimodal structure of the Hercules stream as resulting from multiple resonances with the galactic bar, supporting a slow bar pattern speed.
Contribution
It presents a self-consistent, dynamic N-body model that identifies multiple resonances shaping the Hercules stream, advancing understanding beyond static potential models.
Findings
Hercules stream is dominated by 4:1 and 5:1 resonances.
The model supports a slow bar pattern speed of 40-45 km/s/kpc.
The simulation reveals a trimodal structure of the Hercules stream.
Abstract
Gaia Data Release 2 revealed detailed structures of nearby stars in phase space. These include the Hercules stream, whose origin is still debated. Most of the previous numerical studies conjectured that the observed structures originate from orbits in resonance with the bar, based on static potential models for the Milky Way. We, in contrast, approach the problem via a self-consistent, dynamic, and morphologically well-resolved model, namely a full -body simulation of the Milky Way. Our simulation comprises about 5.1 billion particles in the galactic stellar bulge, bar, disk, and dark-matter halo and is evolved to 10 Gyr. Our model's disk component is composed of 200 million particles, and its simulation snapshots are stored every 10 Myr, enabling us to resolve and classify resonant orbits of representative samples of stars. After choosing the Sun's position in the simulation, we…
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