activity
20112026
most citedThe Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time

568 citations · 8.7k across the 176 of their papers we have counts for

collaborators
Showing 2026Show all

12 papers · 1 filter

astro-ph.GA2026

Impact of Gaia-Sausage-Enceladus merger revealed by a single cosmic clock: thick-to-thin disc transition, gas disc shrinking and bar formation

Natsuki Funakoshi, Daisuke Kawata, Jason L. Sanders +5

Whether the formation of the Galactic bar was connected to the Gaia-Sausage-Enceladus (GSE) merger, the last significant merger experienced by the Milky Way, remains an open questi…

astro-ph.GA2026

Hidden Disruption in Milky Way-like Satellite Galaxy Populations

Gray Thoron, Nora Shipp, Alexander H. Riley +9

Determining whether a satellite galaxy is tidally disrupting from photometric observations alone remains a fundamental challenge in near-field cosmology. Cosmological simulations o…

astro-ph.GA2026

Uncovering the origin of complex velocity distributions in edge-on disc galaxies

Sophie Townson, Marie Martig, Robert J. J. Grand +3

Stellar line-of-sight velocity distributions are a powerful tool for studying galaxy kinematics and formation history, with multiple-peaked LOSVDs often indicating the presence of…

astro-ph.GA2026

Same galaxy, different CGM: how the metal loading of galactic winds regulates the baryon cycle in Milky Way-mass galaxies

Prachi Khatri, Freeke van de Voort, Rebekka Bieri +5

The circumgalactic medium (CGM) is both the reservoir of gas that fuels star formation and galaxy growth, and the repository for the mass, energy, and metals expelled through stell…

astro-ph.GA2026

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters

Pablo Contreras Guerra, Robert J. J. Grand, Marta Reina-Campos +1

Globular clusters (GCs) are long time survivors of galaxy assembly and evolution yet their emergence from an initial cluster population is still poorly constrained. We present the…

astro-ph.GA2026

AGN-driven outflows in dwarf galaxies from cosmological simulations: Internal properties and observational signatures

Elena Arjona-Gálvez, Arianna Di Cintio, Robert J. J. Grand +4

While AGN feedback is a key driver of massive galaxy evolution, its physical properties and observational signatures in the dwarf regime remain poorly understood. We investigate th…

astro-ph.GA2026

Coupling between stellar and HI lopsidedness in Milky Way-type galaxies from the Auriga Superstars cosmological simulations

Arianna Dolfi, Facundo A. Gómez, Rebekka Bieri +5

Lopsidedness is common in disk galaxies, yet its origin and evolution remain unclear. Previous studies typically examined stellar and gas asymmetries separately, but a combined ana…

astro-ph.GA2026

A simulation-based inference of the Milky Way merger history

Andrea Sante, Andreea S. Font, Daisuke Kawata +2

Accreted stars in the Milky Way (MW) preserve information about the progenitor galaxies where they formed in their chemical and kinematic properties. In this study, we use the chem…

astro-ph.GA2026

Winding, Unwinding, Rewinding the Gaia Phase Spiral

Neige Frankel, Marcin Semczuk, Teresa Antoja +10

The Gaia Space Satellite has transformed the field of Galactic Dynamics by collecting 6D phase space information for hundreds of millions of stars. In 2018, it enabled the discover…

astro-ph.GA2026

The diverse nature of spiral arms in the Auriga Superstars cosmological hydrodynamic simulations

Robert J J Grand, Francesca Fragkoudi, Rüdiger Pakmor +4

The dynamical nature and formation mechanism(s) of galactic spiral arms remain long-standing problems in astrophysics. Most theoretical work is based on analytic calculations or id…

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…

astro-ph.GA2026★ 1 cited

Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue

Thomas Tomlinson, Francesca Fragkoudi, Andreia Carrillo +8

The stellar halo of the Milky Way contains the remnants of past accretion events, which could be detectable as substructures in the classical integrals of motion space, such as ene…