The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
arXiv:2510.11284 · doi:10.1093/mnras/stag1090
Abstract
Understanding how past major mergers shaped the Milky Way's present-day structure is a key goal of Galactic archaeology. The Galaxy's chemical and dynamical structure retains the imprint of such events, including a major accretion episode around 8-10 Gyr ago. Recent findings suggest that present-day orbital energy correlates with stellar chemistry and birth location within the merging progenitor galaxy. Using a high-resolution NIHAO-UHD cosmological zoom-in simulation of a Milky Way analogue, we trace the birth positions, ages, and present-day orbits of stars accreted in its last major merger. We show that stars born in the progenitor's core are more tightly bound to the Milky Way and more chemically enriched, while those from the outskirts are less bound and more metal-poor. This supports the Skúladóttir et al. (2025) scenario that accreted progenitor stars of different chemistry were deposited onto different orbital energies as the galaxy was stripped from the outside in, now in a cosmological context. Quantitatively, we measure a metallicity gradient with progenitor birth radius of , demonstrating that abundance patterns retain measurable memory of formation location within the disrupted satellite. This chemodynamical memory is also evident in elemental planes such as [Al/Fe] vs. [Mg/Mn], consistent with gradients in progenitor star formation efficiency. We further show that common integrals-of-motion selections systematically miss stars from the chemically enriched core, biasing reconstructions toward the metal-poor outskirts. Together, our results demonstrate that chemodynamical memory survives the merger and can reconstruct the accreted galaxy's internal structure, while highlighting biases in current selections of accreted stars.
17 pages. Accepted for publication in MNRAS. All code and figures publicly available in GitHub repository at https://github.com/svenbuder/golden_thread_I
References in corpus (54)
- The NumPy array: a structure for efficient numerical computation
- Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
- Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies
- The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
- Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
- Streams, substructures and the early history of the Milky Way
- Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure
- Gaia Data Release 3 Properties and validation of the radial velocities
- The Biggest Splash
- Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
- Evidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy
- From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
- Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances
- Reconstructing the Last Major Merger of the Milky Way with the H3 Survey
- Nitrogen enhancements 440 Myr after the Big Bang: super-solar N/O, a tidal disruption event or a dense stellar cluster in GN-z11?
- Dynamical Relics of the Ancient Galactic Halo
- Origin of chemically distinct discs in the Auriga cosmological simulations
- Halo Substructure in the SDSS-Gaia Catalogue : Streams and Clumps
- The SkyMapper-Gaia RVS view of the Gaia-Enceladus-Sausage -- an investigation of the metallicity and mass of the Milky Way's last major merger
- Chemical Enrichment and Radial Migration in the Galactic Disk -- the origin of the [ Double Sequence
- StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
- Selecting accreted populations: metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations
- Final Targeting Strategy for the SDSS-IV APOGEE-2S Survey
- The GALAH Survey: Chemical tagging and chrono-chemodynamics of accreted halo stars with GALAH+ DR3 and eDR3
- Elevated r-process enrichment in Gaia Sausage and Sequoia
- The Pristine Inner Galaxy Survey (PIGS) I: Tracing the kinematics of metal-poor stars in the Galactic bulge
- The Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
- -process enhancements of Gaia-Enceladus in GALAH DR3
- The SkyMapper DR1.1 Search for Extremely Metal-Poor Stars
- Evidence from Disrupted Halo Dwarfs that -process Enrichment via Neutron Star Mergers is Delayed by Myrs
- Exploring the origin of low-metallicity stars in Milky Way-like galaxies with the NIHAO-UHD simulations
- The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way
- Microarcsecond Astrometry: Science Highlights from Gaia
- The Pristine survey -- XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry
- A fast algorithm for estimating actions in triaxial potentials
- The COMBS survey I: Chemical Origins of Metal-Poor Stars in the Galactic Bulge
- The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
- Metallicity distributions of halo stars: do they trace the Galactic accretion history?
- The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
- The stellar halo in Local Group Hestia simulations II. The accreted component
- A first estimate of the Milky Way dark matter halo spin
- The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
- Exploring the chemodynamics of metal-poor stellar populations
- Tracing birth properties of stars with abundance clustering
- Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift
- Bar-driven dispersal of Galactic substructure
- Evidence of Gaia Enceladus experiencing at least two passages around the Milky Way
- How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations
- From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
- Dead man tells tales: metallicity distribution of the Milky Way stellar halo reveals the past of the GSE progenitor galaxy
- Inferring Galactic Parameters from Chemical Abundances with Simulation-Based Inference
- Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
- Local variations of the radial metallicity gradient in a simulated NIHAO-UHD Milky Way analogue and their implications for (extra-)galactic studies
- A COMPASS to Model Comparison and Simulation-Based Inference in Galactic Chemical Evolution