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From the 1 of 6 linked papers with an AI index.

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6 papers

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…

astro-ph.GA2026

Invariant manifolds in barred galaxy simulations. I. Material density waves

Toni Soler-Terricabras, Mercè Romero-Gómez, Santi Roca-Fà brega

We investigate the dynamical origin and kinematic signatures of spiral structure in an N-body simulation of an isolated barred galaxy, assessing whether invariant manifold theory p…

astro-ph.GA2026

Characterisation of the Clouds' young stellar Bridge using Gaia DR3

Marie Schölch, Óscar Jiménez-Arranz, Mercè Romero-Gómez +1

The interaction between the LMC and SMC (the Clouds) has resulted in prominent tidal features, including an extended bridge of gas and stars connecting the two galaxies. This Bridg…

astro-ph.GA2026

From Gaia to GaiaNIR: II. A new view of the Milky Way bar

Ó. Jiménez-Arranz, M. Schölch, S. Khanna +9

The Milky Way (MW) hosts a central bar whose pattern speed, orientation, and length remain uncertain, largely due to observational biases and selection effects, despite the transfo…

astro-ph.GA2025

Asymmetries in the LMC velocity maps

Marie Schölch, Óscar Jiménez-Arranz, Mercè Romero-Gómez +4

The analysis of precise Gaia DR3 astrometry in the LMC region has revealed asymmetric patterns in the bar quadrupole and the disc outskirts of the LMC in-plane velocity maps. We ai…

astro-ph.GA2025

Dark matter spiral arms in Milky Way-like halos

Marcel Bernet, Pau Ramos, Teresa Antoja +9

The coupling between the dark matter (DM) halo and the stellar disc is a key factor in galactic evolution. While the interaction between structures like the Galactic bar and DM hal…