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Free keywords:
COSMIC-RAY TRANSPORT; ROTATION MEASURES; MAGNETIC-FIELDS;
STAR-FORMATION; GALACTIC WIND; AGN ACTIVITY; HALO; MODEL; GASAstronomy & Astrophysics; galaxies: individual; galaxies: spiral; galaxies: magnetic fields; radio
continuum: galaxies;
Abstract:
CHANG-ES (Continuum Halos in Nearby Galaxies-an EVLA Survey) is an ambitious project to target 35 nearby disk galaxies that are edge-on to the line of sight. The orientation permits both the disk and halo regions to be studied. The observations were initially at 1.5 GHz (L-band) and 6.0 GHz (C-band) in a variety of VLA array configurations, and in all four Stokes parameters, which allowed for spatially resolved images in total intensity plus polarization. The inclusion of polarization is unique to an edge-on galaxy survey and reveals the galaxies' halo magnetic fields. This paper will summarize the results to date, some of which are new phenomena, never seen prior to CHANG-ES. For example, we see that 'X-type' fields, as well as rotation measure reversals, are common features of spiral galaxies. Further observations at 3.0 GHz (S-band) as well as future scientific opportunities will also be described.
