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Context. Radio continuum observations of dwarf–dwarf galaxy mergers, such as NGC 1487, provide crucial insights into magnetic field amplification and cosmic ray (CR) propagation during galactic assembly. Dwarf galaxies are important laboratories for studying cosmic magnetism because they can maintai...

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Autors principals: Taziaux Sam, Basu Aritra, Das Samata, Bomans Dominik J., Galvin Timothy J., Thomson Alec J. M., Heald George H., Kamphuis Peter, Loi Francesca, Stein Michael, Chyży Krysztof T., Riseley Christopher J., Dettmar Ralf-Jürgen, Becker Tjus Julia
Format: Artigo
Idioma:Inglês
Publicat: EDP Sciences 2026-04-01
Col·lecció:Astronomy & Astrophysics
Matèries:
cosmic rays
ism: magnetic fields
ism: structure
galaxy: evolution
galaxies: dwarf
galaxies: individual: ngc 1487
Accés en línia:https://www.aanda.org/articles/aa/full_html/2026/04/aa58420-25/aa58420-25.html
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