Showing 1–20 of 37 results
/ Date/ Name
Aug 22, 2017The Formation of Stellar Clusters in Magnetized, Filamentary Infrared Dark CloudsMay 5, 2008Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: I. Turbulence StatisticsSep 14, 2011Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: III. Implications for Observations and Turbulent EnhancementNov 25, 2021Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC+ and comparing with simulationNov 11, 2011A Stable, Accurate Methodology for High Mach Number, Strong Magnetic Field MHD Turbulence with Adaptive Mesh Refinement: Resolution and Refinement StudiesJun 26, 2015Magnetized Interstellar Molecular Clouds. I. Comparison Between Simulations and Zeeman ObservationsJul 13, 2010Sub-Alfvenic Non-Ideal MHD Turbulence Simulations with Ambipolar Diffusion: II. Comparison with Observation, Clump Properties, and Scaling to Physical UnitsOct 2, 2012Ambipolar Diffusion Heating in Turbulent SystemsMay 31, 2022The Role of Magnetic Fields in the Stability and Fragmentation of Filamentary Molecular Clouds: Two Case Studies at OMC-3 and OMC-4Jan 14, 2019Magnetized interstellar molecular clouds: II. The Large-Scale Structure and Dynamics of Filamentary Molecular CloudsNov 18, 2019The Formation and Evolution of Wide-Orbit Stellar Multiples In Magnetized CloudsNov 17, 2018Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19Apr 16, 2025ALMASOP. Detection of Turbulence-induced Mass Assembly Shocks in Starless CoresJan 6, 2022Magnetic fields in the formation of the first stars.--II ResultsMar 29, 2011Comparing Numerical Methods for Isothermal Magnetized Supersonic TurbulenceMay 10, 2018The TOP-SCOPE survey of PGCCs: PMO and SCUBA-2 observations of 64 PGCCs in the 2nd Galactic QuadrantMar 26, 2018A holistic perspective on the dynamics of G035.39-00.33: the interplay between gas and magnetic fieldsMay 14, 2017ALMA reveals sequential high-mass star formation in the G9.62+0.19 complexJan 28, 2007Two regimes of Turbulent Fragmentation and the stellar IMF from Primordial to Present Day Star FormationMay 18, 2022The Davis-Chandrasekhar-Fermi Method Revisited