A multifrequency radio continuum study of the Magellanic Clouds - I. Overall structure and star formation rates

We present the first low-frequency Murchison Widefield Array (MWA) radio continuum maps of the Magellanic Clouds (MCs), usingmosaics from the GaLactic Extragalactic All-SkyMWA (GLEAM) survey. In this paper, we discuss the overall radio continuum morphology between 76 and 227 MHz and compare them wit...

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Bibliographic Details
Main Authors: For, B., Staveley-Smith, L., Hurley-Walker, Natasha, Franzen, Thomas, Kapinska, A., Filipovic, M., Collier, J., Wu, C., Grieve, K., Callingham, J., Bell, M., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Deshpande, A., Dwarakanath, K., Gaensler, B., Greenhill, L., Hancock, Paul, Hazelton, B., Hindson, L., Johnston-Hollitt, M., Kaplan, D., Lenc, E., Lonsdale, C., McKinley, B., McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Morgan, John, Oberoi, D., Offringa, A., Ord, S., Prabu, T., Procopio, P., Udaya Shankar, N., Srivani, K., Subrahmanyan, R., Tingay, Steven, Wayth, Randall, Webster, R., Williams, Andrew, Williams, C., Zheng, Q.
Format: Journal Article
Published: Oxford University Press 2018
Online Access:http://hdl.handle.net/20.500.11937/73489