Radio synchrotron emission, its polarization and Faraday rotation of the polarization angle
are powerful tools to study the strength and structure of magnetic fields in galaxies …

Radio synchrotron emission, its polarization and its Faraday rotation are powerful tools to
study the strength and structure of magnetic fields in galaxies. Unpolarized emission traces …

Context. Nearby edge-on galaxies showing a synchrotron halo are nearly ideal objects for
studying the transport of cosmic rays (CRs) in galaxies. Among them, the nearby starburst …

We introduce a new survey to map the radio continuum halos of a sample of 35 edge-on
spiral galaxies at 1.5 GHz and 6 GHz in all polarization products. The survey is exploiting the …

Observations of synchrotron radiation and the Faraday rotation of its polarized component
allow us to investigate the magnetic properties of the diffuse interstellar medium in nearby …

Context. Magnetic fields are good tracers of gas compression by shock waves in the
interstellar medium. These can be caused by the interaction of star-formation driven outflows …

Context. The generation and the amplification of magnetic fields in the current cosmological
paradigm are still open questions. The standard theory is based on an early field generation …

Context. The magnetic fields of spiral galaxies are so strong that they cannot qualify as
primordial. Their typical values are over one billion times higher than any value predicted for …

We present self-consistent high-resolution simulations of NGC 4038/4039 (the" Antennae
galaxies") including star formation, supernova feedback, and magnetic fields performed with …

Synchrotron emission, its polarization and its Faraday rotation at radio frequencies of 0.2–10
GHz are powerful tools to study the strength and structure of cosmic magnetic fields …