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...
| المؤلفون الرئيسيون: | , , , , , , , , , , , , , , , , , , , |
|---|---|
| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
American Astronomical Society
2024
|