Showing 21–40 of 271 results
/ Date/ Name
Jul 23, 2019Young star cluster populations in the E-MOSAICS simulationsMay 13, 2020Physical Processes in Star FormationFeb 4, 2020Heart of Darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroidsApr 19, 2021The complex multi-scale structure in simulated and observed emission maps of the proto-cluster cloud G0.253+0.016 (`the Brick')Mar 15, 2021The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clustersMay 3, 2021A scaling relation for the molecular cloud lifetime in Milky Way-like galaxiesApr 7, 2021A Tip of the Red Giant Branch Distance of $22.1 \pm 1.2$ Mpc to the Dark Matter Deficient Galaxy NGC1052-DF2 from 40 Orbits of Hubble Space Telescope ImagingMar 24, 2021The organization of cloud-scale gas density structure: high resolution CO vs. 3.6 $μ$m brightness contrasts in nearby galaxiesSep 2, 2013Comparing molecular gas across cosmic time-scales: the Milky Way as both a typical spiral galaxy and a high-redshift galaxy analogueDec 1, 2014The dynamical evolution of molecular clouds near the Galactic Centre - I. Orbital structure and evolutionary timelineMar 14, 2018Chaos and Variance in Galaxy FormationApr 30, 2018The Maybe Stream: A Possible Cold Stellar Stream in the Ultra-Diffuse Galaxy NGC1052-DF2May 30, 2016Toward gas exhaustion in the W51 high-mass protoclustersJan 10, 2017Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky WayJun 4, 2008Explaining the mass-to-light ratios of globular clustersJan 27, 2025The Formation of Globular ClustersFeb 24, 2017The Varying Mass Distribution of Molecular Clouds Across M83Jun 26, 2017Cloud Scale ISM Structure and Star Formation in M51Oct 7, 2025Context-Aware Inference via Performance Forecasting in Decentralized Learning NetworksJan 8, 2026Unveiling the 3D structure of the central molecular zone from stellar kinematics and photometry: The 50 and 20 km/s clouds