Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Abstract

Within ten nearby (d < 450 pc) Gould Belt molecular clouds we evaluate statistically the relative orientation between the magnetic field projected on the plane of sky, inferred from the polarized thermal emission of Galactic dust observed by Planck at 353 GHz, and the gas column density structures, quantified by the gradient of the column density, $N_H$. The selected regions, covering several degrees in size, are analyzed at an effective angular resolution of 10' FWHM, thus sampling physical scales from 0.4 to 40 pc in the nearest cloud. The column densities in the selected regions range from $N_H\approx 10^{21}$ to $10^{23}$ cm${}^{-2}$, and hence they correspond to the bulk of the molecular clouds. The relative orientation is evaluated pixel by pixel and analyzed in bins of column density using the novel statistical tool called "Histogram of Relative Orientations". Throughout this study, we assume that the polarized emission observed by Planck at 353 GHz is representative of the projected morphology of the magnetic field in each region, i.e., we assume a constant dust grain alignment efficiency, independent of the local environment. Within most clouds we find that the relative orientation changes progressively with increasing $N_H$, from preferentially parallel or having no preferred orientation to preferentially perpendicular. In simulations of magnetohydrodynamic turbulence in molecular clouds this trend in relative orientation is a signature of Alfvénic or sub-Alfvénic turbulence, implying that the magnetic field is significant for the gas dynamics at the scales probed by Planck. We compare the deduced magnetic field strength with estimates we obtain from other methods and discuss the implications of the Planck observations for the general picture of molecular cloud formation and evolution.

28 pages, 20 figures. A&A accepted. Corresponding author: J.D. Soler

References in corpus (18)

• Theory of Star Formation
• Cold Dark Clouds: The Initial Conditions for Star Formation
• Radiative torques: Analytical Model and Basic Properties
• Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
• The Birth of Molecular Clouds: Formation of Atomic Precursors in Colliding Flows
• Studies of regular and random magnetic fields in the ISM: statistics of polarization vectors and the Chandrasekhar-Fermi technique
• A Large Catalog of Accurate Distances to Molecular Clouds from PS1 Photometry
• Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
• The Efficiency of Grain Alignment in Dense Interstellar Clouds: A Reassessment of Constraints from Near Infrared Polarization
• Magnetically Aligned Velocity Anisotropy in the Taurus Molecular Cloud
• Rapid directional alignment of velocity and magnetic field in magnetohydrodynamic turbulence
• Planck intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353 GHz with interstellar polarization in the visible
• Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds
• Grain Alignment in Starless Cores
• Results of SPARO 2003: Mapping Magnetic Fields in Giant Molecular Clouds
• Polarization measurements analysis I. Impact of the full covariance matrix on polarization fraction and angle measurements
• Measuring the Alfvenic Nature of the Interstellar Medium: Velocity Anisotropy Revisited
• Star Forming Regions in Cepheus

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