Magnetism in Nearby Galaxies, Prospects with the SKA, and Synergies with the E-ELT
R. Beck (MPI fuer Radioastronomie, Bonn, Germany)

TL;DR
This paper discusses how upcoming radio telescopes like the SKA will revolutionize the study of magnetic fields in galaxies, revealing their structure, origin, and evolution through advanced polarization and Faraday rotation measurements.
Contribution
It highlights the potential of the SKA and its precursors to perform comprehensive surveys of cosmic magnetic fields and explores synergies with the E-ELT for joint polarimetric observations.
Findings
Ordered magnetic fields exist in various galaxy types.
Faraday rotation reveals large-scale magnetic patterns.
Upcoming surveys will map magnetic fields in detail.
Abstract
Radio synchrotron emission, its polarization and its Faraday rotation are powerful tools to study the strength and structure of interstellar magnetic fields. In the Milky Way, Faraday rotation of the polarized emission from pulsars and background sources indicate that the regular field follows the spiral arms and has one reversal inside the solar radius, but the overall field structure in our Galaxy is still unclear. In nearby galaxies, ordered fields with spiral structure exist in grand-design, barred and flocculent galaxies. The strongest ordered fields (10-15 \muG) are found in interarm regions. Faraday rotation of the diffuse polarized radio emission from the disks of spiral galaxies sometimes reveals large-scale patterns, which are signatures of regular fields generated by a mean-field dynamo. - The SKA and its precursor telescopes will open a new era in the observation of cosmic…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Astronomy and Astrophysical Research
