Showing 1–11 of 11 results
/ Date/ Name
May 12, 2023How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocksFeb 1, 2021Synthetic CO emission and the $X_{\rm CO}$ factor of young molecular clouds: a convergence studyNov 18, 2025Feedback and Star Formation Efficiency in High-Mass Star-Forming RegionsAug 16, 2022RJ-plots: An improved method to classify structures objectivelyJan 20, 2026The Structure of an 80 pc Long Massive FilamentJan 20, 2016Perturbation growth in accreting filamentsFeb 26, 2015Investigating the Global Collapse of Filaments Using Smoothed Particle HydrodynamicsDec 3, 2024Alignment Parameters: Quantifying Dense Core Alignment in Star-forming RegionsDec 10, 2025Can Clump Properties Predict Core Distribution in Star Formation? A Statistical Analysis of MHD SimulationsMay 8, 2022From Bubbles and Filaments to Cores and Disks: Gas Gathering and Growth of Structure Leading to the Formation of Stellar SystemsJan 23, 2024Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-Mass Star-Forming Region NGC2264 : Global Properties and Local Magnetogravitational Configurations