Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA
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DOI: 10.1093/mnras/stw2959
Abstract: Synchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency radio telescope, the Murchison Widefield Array (MWA), we measure the free-free… read more here.
Keywords: synchrotron; galactic synchrotron; hii regions; emissivity ... See more keywords