(abs, pdf) Yan et al., The most massive stars in very young star clusters with a limited mass: Evidence favours significant self-regulation in the star formation processes
(abs, pdf) Kim et al., Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
(abs, pdf) Beckmann et al., Population statistics of intermediate mass black holes in dwarf galaxies using the NewHorizon simulation
(abs, pdf) Rizzuto et al., The growth of intermediate mass black holes through tidal captures and tidal disruption events
(abs, pdf) Beckmann et al., Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
(abs, pdf) Gupta et al., MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
(abs, pdf) Martin-Alvarez et al., The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
(abs, pdf) Phipps et al., Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
(abs, pdf) Trani et al., Growing Black Holes through Successive Mergers in Galactic Nuclei: I. Methods and First Results
(abs, pdf) Snyder et al., Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
(abs, pdf) Riaz et al., Formation of metal-free binaries: Impact of H$_{2}$ line cooling and CIE cooling
(abs, pdf) Santos-Santos et al., Planes of satellites around simulated disk galaxies II: Time-persistent planes of kinematically-coherent satellites in $\Lambda$CDM
(abs, pdf) Chaikin et al., A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
(abs, pdf) Katz et al., PRISM: A Non-Equilibrium, Multiphase Interstellar Medium Model for Radiation Hydrodynamics Simulations of Galaxies
(abs, pdf) Kobayashi et al., Can neutron star mergers alone explain the r-process enrichment of the Milky Way?
(abs, pdf) Andrianomena et al., Emulating cosmological multifields with generative adversarial networks
(abs, pdf) Talei et al., Coupling Semi-Analytic and N-body Galaxies (CoSANG) for cosmological stellar halo simulations I- Methods and the structure of dark matter halos