The radio remnant of SN1993J: an instrumental explanation for the evolving complex structure

We present simulated images of Supernova 1993J at 8.4 GHz using Very Long Baseline Interferometry (VLBI) techniques. A spherically symmetric source model is convolved with realistic uv-plane distributions, together with standard imaging procedures, to assess the extent of instrumental effects on the...

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Bibliographic Details
Main Authors: Heywood, I, Blundell, K, Kloeckner, H, Beasley, A
Format: Journal article
Language:English
Published: 2008