The peculiar mass-loss history of SN 2014C as revealed through AMI radio observations

We present a radio light curve of supernova (SN) 2014C taken with the Arcminute Microkelvin Imager (AMI) Large Array at 15.7 GHz. Optical observations presented by Milisavljevic et al. demonstrated that SN 2014C metamorphosed from a stripped-envelope Type Ib SN into a strongly interacting Type IIn S...

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Hlavní autoři: Anderson, G, Horesh, A, Mooley, K, Rushton, A, Fender, R, Staley, T, Argo, M, Beswick, R, Hancock, P, Pérez-Torres, M, Perrott, Y, Plotkin, R, Pretorius, M, Rumsey, C, Titterington, D
Médium: Journal article
Vydáno: Oxford University Press 2016