The Effects of Radiative Transfer on the PDFs of Molecular MHD Turbulence

Abstract

We study the effects of radiative transfer on the Probability Distribution Functions (PDFs) of simulations of magnetohydrodynamic turbulence in the widely studied ${}^{13}$CO 2-1 transition. We find that the integrated intensity maps generally follow a log-normal distribution, with the cases that have $\tau \approx 1$ best matching the PDF of the column density. We fit a 2D variance-sonic Mach number relationship to our logarithmic PDFs of the form ${\sigma }_{ln(\Sigma /{\Sigma }_0)}^2=A\times ln(1+b^2{\mathcal{M}}_s^2)$ and find that, for parameter $b=1/3$, parameter $A$ depends on the radiative transfer environment. We also explore the variance, skewness, and kurtosis of the linear PDFs finding that higher moments reflect both higher sonic Mach number and lower optical depth. Finally, we apply the Tsallis incremental PDF function and find that the fit parameters depend on both Mach numbers, but also are sensitive to the radiative transfer parameter space, with the $\tau \approx 1$ case best fitting the incremental PDF of the true column density. We conclude that, for PDFs of low optical depth cases, part of the gas is always sub-thermally excited so that the spread of the line intensities exceeds the spread of the underlying column densities and hence the PDFs do not reflect the true column density. Similarly, PDFs of optically thick cases are dominated by the velocity dispersion and therefore do not represent the true column density PDF. Thus, in the case of molecules like carbon monoxide, the dynamic range of intensities, structures observed and consequently, the observable PDFs, are less determined by turbulence and more-often determined by radiative transfer effects.

accepted to ApJ

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• The reliability of observational measurements of column density probability distribution functions
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• Centroid Velocity Statistics of Molecular Clouds
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• The Phase Coherence of Interstellar Density Fluctuations
• Opacity Broadening of ${}^{13}$CO Linewidths and its Effect on the Variance-Sonic Mach Number Relation
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• A Synergy of the Velocity Gradients Technique and the Probability Density Functions for Identifying Gravitational Collapse in Self-Absorbing Media
• Does the HCN/CO ratio trace the star-forming fraction of gas? I. A comparison with analytical models of star formation
• Star formation in IRDC G31.97+0.07
• Constraining cloud parameters using high density gas tracers in galaxies
• Does the HCN/CO ratio trace the star-forming fraction of gas? II. Variations in CO and HCN Emissivity
• Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies