Showing 21–40 of 140 results
/ Date/ Name
Oct 15, 2004Stellar Mass Spectra from Non-Isothermal Gravoturbulent FragmentationJul 22, 2002About the morphology of dwarf spheroidal galaxies and their dark matter contentAug 13, 2014Accretion and magnetic field morphology around Class 0 stage protostellar discsSep 14, 2000Gravitational Collapse in Turbulent Molecular Clouds. II. Magnetohydrodynamical TurbulenceMay 2, 2008Turbulent Mixing in the Interstellar Medium -- an application for Lagrangian Tracer ParticlesJun 22, 2011Magnetic fields during the early stages of massive star formation - I. Accretion and disk evolutionDec 3, 2018Feedback in W49A diagnosed with radio recombination lines and modelsOct 9, 2020Time-Variable Radio Recombination Line Emission in W49AMar 6, 2026Galaxy UV Legacy Project: Survey Description and First Insights Into NGC 4449 Recent History of Star FormationNov 13, 2025ALMAGAL V. Relations between the core populations and the parent clump physical propertiesDec 16, 2008The Clustering Behavior of Pre-Main Sequence Stars in NGC 346 in the Small Magellanic CloudJul 23, 2009Modelling CO formation in the turbulent interstellar mediumOct 28, 2009Solenoidal versus compressive turbulence forcingNov 27, 2023Protostellar chimney flues: are jets and outflows lifting submillimetre dust grains from discs into envelopes?Mar 23, 2023Resolved stellar population properties of PHANGS-MUSE galaxiesJul 24, 2023Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming cloudsJan 8, 2011Collapse, outflows and fragmentation of massive, turbulent and magnetized prestellar barotropic coresMar 9, 2012The Density Variance--Mach Number Relation in Supersonic Turbulence: I. Isothermal, magnetised gasMay 10, 2019WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scalesJun 24, 2021The filamentary structures in the CO emission toward the Milky Way disk