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Smoothed Particle Magnetohydrodynamics Simulations of Protostellar Jets and Turbulent Dynamos

, , , and . (Oct 17, 2013)

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Star Formation in the First Galaxies I: Collapse Delayed by Lyman-Werner Radiation, , , , , and . (2012)cite arxiv:1205.3835Comment: 22 pages, 12 figures.Multiphase Neutral Interstellar Medium: Analyzing Simulation with H I 21cm Observational Data Analysis Techniques, , , , and . (2023)cite arxiv:2309.05000Comment: 21 pages (including appendixes), 15 figures, 3 tables, Submitted to MNRAS, Comments are welcome.Parallel Implementation of Lossy Data Compression for Temporal Data Sets., , , , , , and . HiPC, page 62-71. IEEE Computer Society, (2016)Filament formation in wind-cloud interactions. I. Spherical clouds in uniform magnetic fields, , , , and . (Oct 19, 2015)Nonlinear closures for scale separation in supersonic magnetohydrodynamic turbulence, , , , and . (Jan 28, 2015)On the effective turbulence driving mode of molecular clouds formed in disc galaxies, , , , , and . (Mar 28, 2017)Smoothed Particle Magnetohydrodynamics Simulations of Protostellar Jets and Turbulent Dynamos, , , and . (Oct 17, 2013)The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories, , and . (2019)cite arxiv:1903.01597Comment: Accepted for publication in MNRAS. 10 pages, 7 figures, 2 tables.Unfolding the Laws of Star Formation: The Density Distribution of Molecular Clouds, , and . (2014)cite arxiv:1404.2722Comment: Science (2014) vol. 345. 34 pages.Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1702.03930Comment: 77 pages, 51 figures, 335 equations, submitted to PASA. Code available from https://phantomsph.bitbucket.io/.