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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| Fformat: | Journal article |
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Oxford University Press
2016
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