CAN THE COSMIC RAY DRIVEN DYNAMO MODEL EXPLAIN THE OBSERVATIONS OF THE POLARIZED EMISSION OF EDGE-ON GALAXIES?-Reference-Cited by-同舟云学术

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CAN THE COSMIC RAY DRIVEN DYNAMO MODEL EXPLAIN THE OBSERVATIONS OF THE POLARIZED EMISSION OF EDGE-ON GALAXIES?

Published:2009-02-27 Issue:1 Volume:693 Page:1-7
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Otmianowska-Mazur Katarzyna,Soida Marian,Kulesza-Żydzik Barbara,Hanasz Michał,Kowal Grzegorz

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

1. Magnetic spiral arms in the galaxy NGC6946

2. Rotation and Mass of the Magellanic-Type Galaxy NGC 4631.

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1. Polarization of radio relics in galaxy clusters;Monthly Notices of the Royal Astronomical Society;2019-11-05

2. 3D global simulations of a cosmic-ray-driven dynamo in dwarf galaxies;Astronomy & Astrophysics;2014-02

3. The Fermi bubbles: gamma-ray, microwave and polarization signatures of leptonic AGN jets;Monthly Notices of the Royal Astronomical Society;2013-10-11

4. COSMOLOGICAL MAGNETOHYDRODYNAMIC SIMULATIONS OF GALAXY CLUSTER RADIO RELICS: INSIGHTS AND WARNINGS FOR OBSERVATIONS;The Astrophysical Journal;2013-02-13

5. Interstellar and intergalactic dynamos;Proceedings of the International Astronomical Union;2012-08

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