activity
20222026
most citedCharacterisation of Galactic carbon stars and related stars from Gaia-EDR3

42 citations · 50 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

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

T. Soler-Terricabras, S. Roca-Fàbrega, M. Romero-Gómez

We investigated the origin of the weakening of strong spiral arms in barred galaxies, seeking the physical mechanism responsible for the decline in the fraction of manifold-trapped…

astro-ph.GA2026

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

Toni Soler-Terricabras, Mercè Romero-Gómez, Santi Roca-Fàbrega

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

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★ 4 cited

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★ 4 cited

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…

astro-ph.SR2022★ 42 cited

Characterisation of Galactic carbon stars and related stars from Gaia-EDR3

Carlos Abia, Patrick de Laverny, Merce Romero +1

We extend here a previous investigation on the characteristics of Galactic carbon stars using more accurate EDR3 astrometry measurements. Based on a much larger statistics, we conf…