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Cited article:

Eigenvalue Problem for a Reduced Dynamo Model in Thick Astrophysical Discs

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Open Astronomy 32 (1) (2023)
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Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies

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NGC 5236’s stars as tracers of arms and arm widths in spiral galaxies

E Silva-Villa and X Cano Gómez
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Structure and Features of the Galactic Magnetic-Field Reversals Formation

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https://doi.org/10.1134/S1063772920030014

Synthesizing Observations and Theory to Understand Galactic Magnetic Fields: Progress and Challenges

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https://doi.org/10.3390/galaxies8010004

Evolving galactic dynamos and fits to the reversing rotation measures in the halo of NGC 4631

Alex Woodfinden, R N Henriksen, Judith Irwin and Silvia Carolina Mora-Partiarroyo
Monthly Notices of the Royal Astronomical Society 487 (2) 1498 (2019)
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The origin of the structure of large-scale magnetic fields in disc galaxies

C J Nixon, T O Hands, A R King and J E Pringle
Monthly Notices of the Royal Astronomical Society 477 (3) 3539 (2018)
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Non-linear galactic dynamos and the magnetic Rädler effect

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Probing Magnetic Fields with Square Kilometre Array and its Precursors

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From the Realm of the Nebulae to Populations of Galaxies

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From the Realm of the Nebulae to Populations of Galaxies

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Magnetic spiral arms and galactic outflows

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Non-linear galactic dynamos: a toolbox

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