Showing 1–20 of 50 results
/ Date/ Name
Oct 3, 2023Turbulent Structure In Supernova Remnants G46.8-0.3 And G39.2-0.3 From THOR PolarimetryMar 29, 2017Interpreting the Star Formation Efficiency of Molecular Clouds with Ionising FeedbackJun 1, 2022The signature of large scale turbulence driving on the structure of the interstellar mediumOct 10, 2022Magnetic fields do not suppress global star formation in low metallicity dwarf galaxiesAug 20, 2018Confirmation Of Two Galactic Supernova Remnant Candidates Discovered By THORMar 23, 2026Shaping the diffuse X-ray sky: Structure, Variability and VisibilityAug 31, 2023The Orion-Taurus ridge: a synchrotron radio loop at the edge of the Orion-Eridanus superbubbleJan 19, 2023On the distribution of the Cold Neutral Medium in galaxy discsMay 20, 2022The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emissionJul 21, 2020Synthetic observations of spiral arm tracers of a simulated Milky Way analogApr 29, 2024Faraday tomography of LoTSS-DR2 data: II. Multi-tracer analysis in the high-latitude outer GalaxyMar 1, 2024Cloud properties across spatial scales in simulations of the interstellar mediumFeb 4, 2025Introducing the Rhea simulations of Milky-Way-like galaxies I: Effect of gravitational potential on morphology and star formationMar 5, 2025The role of turbulence in setting the phase of the ISM and implications for the star formation rateSep 30, 2024Local HI Absorption towards the Magellanic Cloud foreground using ASKAPOct 22, 2024A 3D Model of the Local Bubble's Magnetic Field: Insights from Dust and Starlight PolarizationJul 14, 2025The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulationsSep 11, 2019Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structureJul 2, 2020Detailed 3D structure of OrionA in dust with Gaia DR2Oct 2, 2020The relative orientation between the magnetic field and gas density structures in non-gravitating turbulent media