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Cosmic magnetism in centimeter- and meter-wavelength radio astronomy

Author(s)
Akahori, TakuyaNakanishi, HiroyukiSofue, YoshiakiFujita, YutakaIchiki, KiyotomoIdeguchi, ShinsukeKameya, OsamuKudoh, TakahiroKudoh, YukiMachida, MamiMiyashita, YoshimitsuOhno, HiroshiOzawa, TakeakiTakahashi, KeitaroTakizawa, MotokazuYamazaki, Dai G.
Issued Date
2018-01
DOI
10.1093/pasj/psx123
URI
https://scholarworks.unist.ac.kr/handle/201301/23810
Fulltext
https://academic.oup.com/pasj/article/70/1/R2/4770210
Citation
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, v.70, no.1, pp.R21 - R244
Abstract
The magnetic field is ubiquitous in the universe. Though it plays an essential role in various astrophysical phenomena, its real origin and evolution are poorly known. This article reviews the understanding of the latest research concerning 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 is concentrated in the achievements that have been provided by centimeter- and meter-wavelength radio observations. The article also introduces various methods for analyzing linear polarization data, including synchrotron radiation, Faraday rotation, depolarization, and Faraday tomography.
Publisher
OXFORD UNIV PRESS
ISSN
0004-6264
Keyword (Author)
magnetic fieldsmethods: observationalpolarizationradio continuum: generaltechniques: polarimetric
Keyword
ACTIVE GALACTIC NUCLEIPULSAR ROTATION MEASURESSUPERMASSIVE BLACK-HOLEX-RAY-EMISSIONMICROWAVE BACKGROUND ANISOTROPIESEXTRAGALACTIC FARADAY-ROTATIONNEAR-INFRARED POLARIMETRYBIG-BANG NUCLEOSYNTHESISSQUARE KILOMETER ARRAYMOLECULAR CLOUD CORES

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