Showing 1–20 of 21 results
/ Date/ Name
Dec 28, 2021Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populationsJan 7, 2021Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematicsJun 13, 2018A new model for the multiple stellar populations within Terzan 5Feb 13, 2023Peeking beneath the precision floor -- II. Probing the chemo-dynamical histories of the potential globular cluster siblings, NGC 288 and NGC 362Nov 13, 2024$S^5$: New insights from deep spectroscopic observations of the tidal tails of the globular clusters NGC 1261 and NGC 1904Feb 5, 20243D NLTE Lithium abundances for late-type stars in GALAH DR3Apr 8, 2025Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first starsJun 3, 2025Optical spectroscopic signatures of the red giant evolutionary stateOct 17, 2025Spectroscopic Follow-up of Young High-$α$ Dwarf Star Candidates: Still Likely Genuinely YoungJan 10, 2025The GALAH survey: Improving chemical abundances using star clustersOct 26, 2022Peeking beneath the precision floor I: metallicity spreads and multiple elemental dispersions in the globular clusters NGC 288 and NGC 362Jan 4, 2024Multiple Populations and a CH Star Found in the 300S Globular Cluster Stellar StreamJan 22, 2025Formation of massive star clusters with and without iron abundance spreads in a dwarf galaxy mergerOct 22, 2024Chemical Abundances in the Leiptr Stellar Stream: A Disrupted Ultra-faint Dwarf Galaxy?Oct 13, 2025The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue I: A golden thread through time and spaceSep 20, 2023Galaxy archaeology for wet mergers: Globular cluster age distributions in the Milky Way and nearby galaxiesMay 14, 2024The ratio of [Eu/$α$] differentiates accreted/in-situ Milky Way stars across metallicities, as indicated by both field stars and globular clustersOct 23, 2025The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue II: Were Splash stars heated or already born hot?Jun 18, 2025Chemical Abundances in the Metal-Poor Globular Cluster ESO 280-SC06: A Formerly Massive, Tidally Disrupted Globular ClusterFeb 22, 2024Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models