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Characterizing the Turbulent Properties of the Starless Molecular Cloud MBM16
Nickolas M. Pingel, Snezana Stanimirovic, J. E. G. Peek +13
We investigate turbulent properties of the non-star-forming, translucent molecular cloud, MBM16 by applying the statistical technique of a two-dimensional spatial power spectrum (S…
Observational Diagnostics for Two-Fluid Turbulence in Molecular Clouds As Suggested by Simulations
Chad D. Meyer, Dinshaw S. Balsara, Blakesley Burkhart +1
We present high resolution simulations of two-fluid (ion-neutral) MHD turbulence with resolutions as large as 512^3. The simulations are supersonic and mildly sub-Alfvenic, in keep…
The Turbulence Power Spectrum in Optically Thick Interstellar Clouds
Blakesley Burkhart, A. Lazarian, V. Ossenkopf +1
The Fourier power spectrum is one of the most widely used statistical tools to analyze the nature of magnetohydrodynamic turbulence in the interstellar medium. Lazarian & Pogosyan…
The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence
Blakesley Burkhart, V. Ossenkopf, A. Lazarian +1
We study the effects of radiative transfer on the Probability Distribution Functions (PDFs) of simulations of magnetohydrodynamic turbulence in the widely studied CO 2-1 tra…