collaborators

14 papers

astro-ph.GA2026

Dissecting the 3D chemo-dynamical structures of NGC 1381: a galaxy hosting an ancient slow bar with an accreted bulge and thick disc

Yunpeng Jin, Ling Zhu, Shude Mao +4

We applied the barred population-orbit superposition method developed in \citet{Jin2025a,Jin2025b} to construct 3D chemo-dynamical models for the barred S0 galaxy NGC~1381 in the F…

astro-ph.GA2026

The GECKOS survey: Resolving the molecular and ionised gas in the galactic outflow of ESO~484-036

J. Hernández-Yévenes, D. B. Fisher, B. Mazzilli Ciraulo +20

We present a spatially resolved, multiphase study of the outflow in the edge-on starburst galaxy ESO~484-036 from the GECKOS survey, combining VLT/MUSE H and ALMA CO(10) obs…

astro-ph.GA2026

The Radial and Vertical Structure of Molecular Gas in the Edge-On Galaxy NGC 4565

Grace Krahm, Adam K. Leroy, Jiayi Sun +11

We present high-resolution (0.94" 55 pc) ALMA CO(2-1) and 13CO(2-1) observations of the highly inclined (i~87.5 deg) galaxy NGC 4565 covering out to galactocentric radius…

astro-ph.GA2026

The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history

J. P. Bernaldez, I. Minchev, B. Ratcliffe +7

Reconstructing the star formation history (SFH) of disk galaxies is central to understanding their growth and evolution, yet such estimates can be strongly biased by stellar radial…

astro-ph.GA2026

The GECKOS Survey: Extraplanar ionised gas in star-forming galaxies from eDIG to galaxy-scale winds

R. Elliott, D. B. Fisher, B. Mazzilli Ciraulo +19

We map the extraplanar gas, with 50-200 pc resolution, in nine star-forming galaxies using Multi-Unit Spectroscopic Explorer (MUSE) observations from the GECKOS VLT Large Pro…

astro-ph.GA2026

What drives bar rotation? The effect of internal properties and galaxy interactions on bar pattern speeds

Alex Merrow, Francesca Fragkoudi, Rob J. J. Grand +1

One of the main properties of galactic bars is their rotation (or pattern) speed, which is driven by both internal galactic properties, as well as external interactions. To assess…