Extragalactic magnetism with SOFIA (SALSA Legacy Program). VII. A tomographic view of far-infrared and radio polarimetric observations through MHD simulations of galaxies

The structure of magnetic fields in galaxies remains poorly constrained, despite the importance of magnetism in the evolution of galaxies. Radio synchrotron and far-infrared (FIR) polarization and polarimetric observations are the best methods to measure galactic scale properties of magnetic fields...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Martin-Alvarez, S, Lopez-Rodriguez, E, Dacunha, T, Clark, SE, Borlaff, AS, Beck, R, Montero, FR, Jung, SL, Devriendt, J, Slyz, A, Roman-Duval, J, Ntormousi, E, Tahani, M, Subramanian, K, Dale, DA, Marcum, PM, Tassis, K, del Moral-Castro, I, Tram, LN, Jarvis, MJ
Aineistotyyppi: Internet publication
Kieli:English
Julkaistu: 2023

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