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CHANG-ES XXIII: Influence of a galactic wind in NGC 5775
[article]
2021
arXiv
pre-print
We present new radio continuum images of the edge-on starburst galaxy NGC 5775, from LOFAR (140 MHz) and the Karl G. Jansky Very Large Array CHANG-ES survey (1500 MHz). We trace the non-thermal radio halo up to 13 kpc from the disc, measuring the non-thermal spectral index and estimating the total equipartition magnetic field strength (≈13μG in the disc and ≈7μG above the plane). The radio halo has a similar extent at both frequencies, displays evidence for localized cosmic ray streaming
arXiv:2109.12267v1
fatcat:sqk7hoxhtnc6nbbbdfau6lavki