Galactic synchrotron emissivity measurements between 250° MWA

Su, H., Hurley-Walker, N., Jackson, C. A., McClure-Griffiths, N. M., Tingay, S. J., Hindson, L., Hancock, P., Wayth, R. B., Gaensler, B. M., Staveley-Smith, L., Morgan, J., Johnston-Hollitt, M., Lenc, E., Bell, M. E., Callingham, J. R., Dwarkanath, K. S., For, B. Q., Kapińska, A. D., McKinley, B., Offringa, A. R., Procopio, P., Wu, C. and Zheng, Q. (2017) Galactic synchrotron emissivity measurements between 250° MWA. Monthly Notices of the Royal Astronomical Society (MNRAS), 465 (3). pp. 3163-3174. ISSN 0035-8711
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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 absorption of this Galactic synchrotron emission by intervening HII regions along the line of sight. These absorption measurements allow us to calculate the Galactic cosmic-ray electron emissivity behind and in front of 47 detected HII regions in the region $250^\circ


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