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- W2022125139 endingPage "59" @default.
- W2022125139 startingPage "59" @default.
- W2022125139 abstract "In this work, we present the mass and magnetic distributions found in a recent Adaptive Mesh Refinement (AMR) MHD simulation of supersonic, sa, self gravitating turbulence. Powerlaw tails are found in both volume density and magnetic field probability density functions, with $P(rho) propto rho^{-1.67}$ and $P(B)propto B^{-2.74}$. A power law is also found between magnetic field strength and density, with $Bpropto rho^{0.48}$, throughout the collapsing gas. The mass distribution of gravitationally bound cores is shown to be in excellent agreement with recent observation of prestellar cores. The mass to flux distribution of cores is also found to be in excellent agreement with recent Zeeman splitting measurements." @default.
- W2022125139 created "2016-06-24" @default.
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- W2022125139 creator A5085942365 @default.
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- W2022125139 date "2011-03-23" @default.
- W2022125139 modified "2023-10-06" @default.
- W2022125139 title "MASS AND MAGNETIC DISTRIBUTIONS IN SELF-GRAVITATING SUPER-ALFVÉNIC TURBULENCE WITH ADAPTIVE MESH REFINEMENT" @default.
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- W2022125139 doi "https://doi.org/10.1088/0004-637x/731/1/59" @default.
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