#galactic dynamics

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4 papers match

astro-ph.GA2026

Invariant manifolds in barred galaxy simulations. III. Self-regulated weakening of strong spiral arms

T. Soler-Terricabras, S. Roca-Fà brega, M. Romero-Gómez

The paper investigates why strong spiral arms in barred galaxies weaken, showing that self‑gravitating spirals shift the galaxy’s Lagrangian points, disrupting invariant‑manifold d…

#barred galaxies#spiral arms#invariant manifolds#galactic dynamics
astro-ph.GA2026

On the current status of tidal tails of Galactic open clusters

Tahereh Ramezani, Nikola Faltova, Prapti Mondal +4

The paper reviews recent observations and theories of tidal tails around Galactic open clusters, emphasizing how Gaia data and different detection methods shape our understanding o…

#open clusters#tidal tails#galactic dynamics#gaia data
astro-ph.GA2026

Chemodynamical evidence of the HR 1614 moving group as a bar resonance

Andreas J. Koch-Hansen, Vladislav Gulaev, Dominik H. Plonka +4

The study combines high‑resolution spectroscopy of six HR 1614 moving‑group stars with orbital frequency analysis to show that the group’s diverse ages and chemical patterns are be…

#moving groups#galactic bar resonance#stellar chemistry#galactic dynamics
astro-ph.GA2026

A differentiable hydrodynamical approach to the Milky Way bar pattern speed with CO longitude--velocity data

Junichi Baba, Kohei Hattori

The paper presents a differentiable hydrodynamical framework that simulates gas flow in the Milky Way’s barred potential and uses CO longitude‑velocity data to constrain the bar’s…

#galactic dynamics#milky way#hydrodynamical simulations#bar pattern speed