Radio broadband visualization of global three-dimensional magnetohydrodynamical simulations of spiral galaxies – I. Faraday rotation at 8 GHz-Reference-Cited by-同舟云学术

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Radio broadband visualization of global three-dimensional magnetohydrodynamical simulations of spiral galaxies – I. Faraday rotation at 8 GHz

Published:2018-07-06 Issue:1 Volume:480 Page:17-25
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Machida M¹,Akahori T²³,Nakamura K E³,Nakanishi H²³³,Haverkorn M³

Affiliation:

1. Department of Physics, Faculty of Sciences, Kyushu University, 744 Motooka, Nishi-ku, Fukuoka, 819-0395, Japan

2. Graduate School of Science and Engineering, Kagoshima University, Korimoto 1-21-35, Kagoshima 890-0065, Japan

3. Department of Astrophysics / IMAPP, Radboud University Nijmegen, PO Box 9010, NL-6500 GL Nijmegen, the Netherlands

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/1/17/25231081/sty1799.pdf

Reference33 articles.

1. SIMULATED FARADAY ROTATION MEASURES TOWARD HIGH GALACTIC LATITUDES

2. Exploring the intergalactic magnetic field by means of Faraday tomography

3. Optimum frequency band for radio polarization observations

4. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

5. Magnetism in the spiral galaxy NGC 6946: magnetic arms, depolarization rings, dynamo modes, and helical fields

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1. Pseudo-observation of spiral galaxies in the radio band to verify depolarization models;Publications of the Astronomical Society of Japan;2023-01-06

2. Faraday Depolarization Effects in Spiral Galaxies;Galaxies;2019-01-12

3. Strategy to Explore Magnetized Cosmic Web with Forthcoming Large Surveys of Rotation Measure;Galaxies;2018-11-16

4. Radio broad-band visualization of global three-dimensional magnetohydrodynamical simulations of spiral galaxies – II. Faraday depolarization from 100 MHz to 10 GHz;Monthly Notices of the Royal Astronomical Society;2018-10-31

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