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...

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Bibliografski detalji
Glavni autori: Martin-Alvarez, S, Lopez-Rodriguez, E, Dacunha, T, Clark, SE, Borlaff, AS, Beck, R, Rodríguez Montero, F, Jung, SL, Devriendt, J, Slyz, A, Roman-Duval, JC, Ntormousi, E, Tahani, M, Subramanian, K, Dale, DA, Marcum, PM, Tassis, K, del Moral-Castro, I, Tram, LN, Jarvis, MJ
Format: Journal article
Jezik:English
Izdano: American Astronomical Society 2024

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