Filaments and striations: anisotropies in observed, supersonic, highly-magnetised turbulent clouds

TL;DR

This study systematically analyzes anisotropies in magnetized, supersonic turbulent molecular clouds using simulations, revealing how magnetic field strength and turbulence influence filament and striation formations.

Contribution

It provides a detailed characterization of anisotropies in molecular clouds, linking magnetic and turbulent parameters to observable structural features.

Findings

Strong magnetic fields lead to anisotropy dominated by striations aligned with the field.

High-density filaments form perpendicular to magnetic fields at higher turbulence levels.

Turbulence and magnetic field strength jointly determine cloud morphology.

Abstract

Stars form in highly-magnetised, supersonic turbulent molecular clouds. Many of the tools and models that we use to carry out star formation studies rely upon the assumption of cloud isotropy. However, structures like high-density filaments in the presence of magnetic fields, and magnetosonic striations introduce anisotropies into the cloud. In this study we use the two-dimensional (2D) power spectrum to perform a systematic analysis of the anisotropies in the column density for a range of Alfv\'en Mach numbers ($\mathcal{M}_A=0.1$--$10$) and turbulent Mach numbers ($\mathcal{M}=2$--$20$), with 20 high-resolution, three-dimensional (3D) turbulent magnetohydrodynamic simulations. We find that for cases with a strong magnetic guide field, corresponding to $\mathcal{M}_A<1$, and $\mathcal{M}\lesssim 4$, the anisotropy in the column density is dominated by thin striations aligned with the magnetic field, while for $\mathcal{M}\gtrsim 4$ the anisotropy is significantly changed by high-density filaments that form perpendicular to the magnetic guide field. Indeed, the strength of the magnetic field controls the degree of anisotropy and whether or not any anisotropy is present, but it is the turbulent motions controlled by $\mathcal{M}$ that determine which kind of anisotropy dominates the morphology of a cloud.