# The Transition from a Lognormal to a Power-Law Column Density   Distribution in Molecular Clouds: An Imprint of the Initial Magnetic Field   and Turbulence

**Authors:** Sayantan Auddy, Shantanu Basu, and Takahiro Kudoh

arXiv: 1907.09783 · 2019-08-14

## TL;DR

This paper presents a theory and simulations showing how the transition point in the column density distribution of molecular clouds depends on initial magnetic field strength and turbulence, revealing insights into cloud evolution.

## Contribution

The authors develop an analytic model linking the transition column density to initial magnetic and turbulent conditions, supported by MHD simulations.

## Key findings

- Transition column density increases with magnetic field and turbulence strength.
- Analytic expression relates $\,m \Sigma_{TP}\, $ to initial Mach number and plasma beta.
- $\,m \Sigma_{TP}\, $ indicates the boundary for gravitational collapse.

## Abstract

We introduce a theory for the development of a transitional column density $\Sigma_{\rm TP}$ between the lognormal and the power-law forms of the probability distribution function (PDF) in a molecular cloud. Our turbulent magnetohydrodynamic simulations show that the value of $\Sigma_{\rm TP}$ increases as the strength of both the initial magnetic field and turbulence increases. We develop an analytic expression for $\Sigma_{\rm TP}$ based on the interplay of turbulence, a (strong) magnetic field, and gravity. The transition value $\Sigma_{\rm TP}$ scales with $\mathcal{M}^2_{\rm 0}$, the square of the initial sonic Mach number, and $\beta_{0}$, the initial ratio of gas pressure to magnetic pressure. We fit the variation of $\Sigma_{\rm TP}$ among different model clouds as a function of $\mathcal{M}^2_{\rm 0} \beta_{0}$, or equivalently the square of the initial Alfv\'enic Mach number $\mathcal{M}^2_{\rm A0}$. This implies that the transition value $\Sigma_{\rm TP}$ is an imprint of cloud initial conditions and is set by turbulent compression of a magnetic cloud. Physically, the value of $\Sigma_{\rm TP}$ denotes the boundary above which the mass-to-flux ratio becomes supercritical and gravity drives the evolution.

## Full text

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## Figures

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## References

44 references — full list in the complete paper: https://tomesphere.com/paper/1907.09783/full.md

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Source: https://tomesphere.com/paper/1907.09783