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Using The Velocity Anisotropy Technique To Investigate Interstellar Magnetohydrodynamic Turbulence
2016
Zenodo
Magnetohydrodynamic (MHD) turbulence in the interstellar medium (ISM) influences star formation and subsequently the way our Galaxy evolves. Direct observations of magnetic fields for studying MHD turbulence can be difficult and costly to obtain; as an alternative, we explore a technique called velocity anisotropy to probe MHD turbulence. We apply the velocity anisotropy technique (VAT) in CO radiative transfer MHD simulations for the first time and also to non-synthetic observations for the
doi:10.5281/zenodo.50082
fatcat:jmhbrrr7sjccne6nte6i5pfuee