Cosmic Magnetism in Centimeter and Meter Wavelength Radio Astronomy

Abstract

Magnetic field is ubiquitous in the Universe and it plays essential roles in various astrophysical phenomena, yet its real origin and evolution are poorly known. This article reviews current understanding of magnetic fields in the interstellar medium, the Milky Way Galaxy, external galaxies, active galactic nuclei, clusters of galaxies, and the cosmic web. Particularly, the review concentrates on the achievements that have been provided by centimeter and meter wavelength radio observations. The article also introduces various methods to analyze linear polarization data, including synchrotron radiation, Faraday rotation, depolarization, and Faraday tomography.

arXiv comment40 pages, 16 figures, accepted for publication in PASJ

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• Baryon Loading of AGN Jets Mediated by Neutrons
• MHD Turbulence and Cosmic Ray Reacceleration in Galaxy Clusters
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• Stability Analysis for Cosmic-Ray Heating of Cool Cores in Galaxy Clusters
• Simulated Faraday Rotation Measures toward High Galactic Latitudes
• Magnetic fields of active galactic nuclei and quasars with polarized broad H-alpha lines
• Temperature and Density in the Foot Points of the Molecular Loops in the Galactic Center; Analysis of Multi-J Transitions of 12CO(J=1-0, 3-2, 4-3, 7-6), 13CO(J=1-0) and C18O(J=1-0)
• The magnetic fields of large Virgo cluster spirals: Paper II
• Faraday dispersion functions of galaxies
• Faraday caustics: Singularities in the Faraday spectrum and their utility as probes of magnetic field properties
• Similarity between the Molecular Loops in the Galactic Center and the Solar Chromospheric Arch Filaments
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• X-ray Spectroscopy of Clusters of Galaxies
• Investigating the hard X-ray emission from the hottest Abell cluster A2163 with Suzaku
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• Constraint of Non-thermal X-ray Emission from the On-going Merger Cluster Abell 3376 with Suzaku
• Discovery of Molecular Loop 3 in the Galactic Center: Evidence for a Positive-Velocity Magnetically Floated Loop towards $L=355^{\circ }-359^{\circ }$
• Generation of Magnetic Field on the Accretion Disk around a Proto-First-Star
• High Excitation Molecular Gas in the Galactic Center Loops; 12CO(J =2-1 and J =3-2) Observations
• CMB with the background primordial magnetic field
• Testing Galactic Magnetic Field Models using Near-Infrared Polarimetry
• Performance test of RM CLEAN and its evaluation with chi-square value
• The Primordial Origin Model of Magnetic Fields in Spiral Galaxies
• Constraining Galactic Magnetic Field Models with Starlight Polarimetry
• Cross-Correlation of Diffuse Synchrotron and Large-Scale Structures
• No Microwave Flare of Sagittarius A* around the G2 Periastron Passing
• A Relativistic Electron-Positron Outflow from a Tepid Fireball
• Study of Vertical Magnetic Field in Face-on Galaxies using Faraday Tomography
• The connection between radio halos and cluster mergers and the statistical properties of the radio halo population
• Formation of gaseous arms in barred galaxies with dynamically important magnetic field : 3D MHD simulations
• Evolution of the cosmic matter density field with a primordial magnetic field
• Seeking large-scale magnetic fields in a pure-disk dwarf galaxy NGC 2976
• Effects of a primordial magnetic field with log-normal distribution on the cosmic microwave background
• The Magnetic Field of the H~II Region NGC 6334A
• A Possible Time-Delayed Brightening of the Sgr A* Accretion Flow after the Pericenter Passage of G2 Cloud
• Three-Dimensional Aquila Rift: Magnetized HI Arch Anchored by Molecular Complex
• New limits on the generation of magnetic field
• Conversion from linear to circular polarization in FPGA
• Radio SNRs in the Magellanic Clouds as probes of shock microphysics

Cited by in corpus (27)

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• The Galactic Plane Infrared Polarization Survey (GPIPS): Data Release 4
• Spectral properties of magnetohydrodnamic turbulence revealed by polarization synchrotron emission with Faraday rotation
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• Discovery of Kolmogorov-like Magnetic Energy Spectrum in Tycho's Supernova Remnant by Two-point Correlations of Synchrotron Intensity
• Science Pipelines for the Square Kilometre Array
• An Iterative Reconstruction Algorithm for Faraday Tomography
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• On the Potential of Faraday Tomography to Identify Shock Structures in Supernova Remnants
• Trans-Alfvenic Magnetohydrodynamic Turbulence in the Vicinity of Supernova Remnant Cassiopeia-A Shocks
• Magnetic field vector maps of nearby spiral galaxies
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• Magnetic field generation by charge exchange in a supernova remnant in the early universe