activity
20242026
most citedEfficient and accurate force replay in cosmological-baryonic simulations

12 citations · 21 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2026

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators

Cecilia Steel, Andrew Wetzel, Rori Kang +3

Stars can radially redistribute (migrate) within galactic disks. The degree to which this occurs as dynamically `cold' (preserves orbital eccentricity) or `hot' (increases eccentri…

astro-ph.GA2026

No Stream Left Unscathed: The imprint of a host galaxy

Arpit Arora, Peter S. Ferguson, Jacob Nibauer +11

Stellar streams from disrupted globular clusters are excellent probes of dark matter (DM) subhalos. Observed Milky Way streams display a remarkable diversity of features: spurs, ga…

astro-ph.GA2026

Radial redistribution of stellar orbits in FIRE simulations of Milky-Way-mass galaxies

Matthew A. Bellardini, Fiona McCluskey, Andrew Wetzel +3

A central question in galactic dynamics and galactic archeology is: how much do the orbits of stars redistribute (migrate) after birth? We use the FIRE-2 cosmological zoom-in simul…

astro-ph.GA2026

The origin of strong -element bimodalities in FIRE simulations of Milky Way-mass galaxies

Megan Barry, Andrew Wetzel, Sarah Loebman +2

One of the Milky Way's characteristic features is a strongly bimodal distribution of -process elements, such as Mg, at fixed [Fe/H] in stellar abundances. We examine patterns in…

astro-ph.GA2025

Understanding the Origin and Dynamical Evolution of the Unique Open Star Cluster Berkeley 20 using FIRE Simulations

Alessa I. Wiggins, Jamie R. Quinn, Micah Oeur +11

Open clusters (OCs) act as key probes that can be leveraged to constrain the formation and evolution of the Milky Way (MW)'s disk, as each has a unique chemical fingerprint and wel…

astro-ph.GA2025

Testing the Stellar Feedback-driven Breathing Mode in Low-mass Galaxies with Gas Kinematics

Yifei Luo, Joseph Wick, Alexie Leauthaud +7

Hydrodynamic simulations have proposed that stellar feedback and bursty star-formation can produce dark matter cores in low-mass galaxies. A key prediction is that feedback-driven…

astro-ph.GA2025

Spiral Structure Properties, Dynamics, and Evolution in MW-mass Galaxy Simulations

J. R. Quinn, S. R. Loebman, K. J. Daniel +8

The structure of spiral galaxies is essential to understanding the dynamics and evolution of disk galaxies; however, the precise nature of spiral arms remains uncertain. Two challe…

astro-ph.GA2025★ 2 cited

Stellar Velocity Dispersion versus Age: Consistency across Observations and Simulations, with the Milky Way as an Outlier

Fiona McCluskey, Andrew Wetzel, Sarah Loebman +1

Within disk galaxies, the velocity dispersion, , of stars increases with age, , as measured in the Milky Way (MW) and nearby galaxies. This relation provides a key window int…

astro-ph.GA2025

Effect of gas accretion on -element bimodality in Milky Way-mass galaxies in the FIRE-2 simulations

Hanna Parul, Jeremy Bailin, Sarah R. Loebman +3

We analyse the stellar distributions on the [Fe/H]-[Mg/Fe] plane for 11 Milky Way-mass galaxies from the FIRE-2 cosmological baryonic zoom-in simulations. Alpha-element bimodality,…

astro-ph.GA2024★ 1 cited

Inside-out versus Upside-down: The Origin and Evolution of Metallicity Radial Gradients in FIRE Simulations of Milky Way-mass Galaxies and the Essential Role of Gas Mixing

Russell L. Graf, Andrew Wetzel, Jeremy Bailin +1

Within the Milky Way (MW), younger stellar populations exhibit steeper (more negative) metallicity radial gradients; the origin of this trend remains debated. The FIRE-2 cosmologic…

astro-ph.GA2024

Strong Chemical Tagging in FIRE: Intra and Inter-Cluster Chemical Homogeneity in Open Clusters in Milky Way-like Galaxy Simulations

Binod Bhattarai, Sarah R. Loebman, Melissa K. Ness +4

Open star clusters are the essential building blocks of the Galactic disk; "strong chemical tagging" - the premise that all star clusters can be reconstructed given chemistry infor…

astro-ph.GA2024★ 12 cited

Efficient and accurate force replay in cosmological-baryonic simulations

Arpit Arora, Robyn Sanderson, Christopher Regan +8

We construct time-evolving gravitational potential models for a Milky Way-mass galaxy from the FIRE-2 suite of cosmological-baryonic simulations using basis function expansions. Th…

astro-ph.GA2024★ 5 cited

The imprint of dark matter on the Galactic acceleration field

Arpit Arora, Robyn E. Sanderson, Sukanya Chakrabarti +6

Measurements of the accelerations of stars enabled by time-series extreme-precision spectroscopic observations, from pulsar timing, and from eclipsing binary stars in the Solar Nei…

astro-ph.GA2024★ 1 cited

Spatial Variations of Stellar Elemental Abundances in FIRE Simulations of Milky Way-Mass Galaxies: Patterns Today Mostly Reflect Those at Formation

Russell L. Graf, Andrew Wetzel, Matthew A. Bellardini +1

Spatial patterns of stellar elemental abundances encode rich information about a galaxy's formation history. We analyze the radial, vertical, and azimuthal variations of metals in…