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...

詳細記述

書誌詳細
主要な著者: 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
フォーマット: Journal article
言語:English
出版事項: American Astronomical Society 2024