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20242026
most citedMUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts

2 citations · 2 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20262 cited

MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts

B. I. Ciocan, N. F. Bouché, J. Fensch +5

The radial acceleration relation (RAR) is a tight empirical correlation between the observed radial acceleration (a_tot) and the baryonic radial acceleration (a_bar) measured acros…

gr-qc2026

Improved constraints on modified Newtonian gravity from Cassini radio tracking data

R. S. Park, A. Hees, B. Famaey +2

We report an updated constraint on the Solar System quadrupole parameter , which encodes the external field effect predicted by modified gravity versions of the modified Newto…

astro-ph.GA2025

Asymmetries in stellar streams induced by a galactic merger

Claire Guillaume, Florent Renaud, Nicolas F. Martin +6

Stellar streams are sensitive to perturbations from, e.g., giant molecular clouds, bars and spiral arms, infalling dwarf galaxies, or globular clusters which can imprint gaps, clum…

astro-ph.GA2025

A non-axisymmetric potential for the Milky Way disk

Y. R. Khalil, B. Famaey, G. Monari +9

We provide a purely dynamical global map of the non-axisymmetric structure of the Milky Way disk. For this, we exploit the information contained within the in-plane motions of disk…

astro-ph.GA2024

Exploring the impact of a rapidly decelerating bar on transforming bulge orbits into disc-like orbits

Chengdong Li, Zhen Yuan, Giacomo Monari +7

The most metal-poor tail of the Milky Way ([Fe/H] 2.5) contains a population of stars with very prograde planar orbits, which is puzzling in both their origin and evoluti…