By J.M. Marcaide, Kurt Weiler
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Extra resources for Cosmic Explosions: On the 10th Anniversary of SN1993J (IAU Colloquium 192) (Springer Proceedings in Physics)
M. Marcaide Fig. 2. Observed spectral index, α, of SN1993J from t ∼70 days up to t=2820 days, as obtained from ﬁtting at each epoch the available VLA data to a synchrotron spectrum, partially suppressed by free-free absorption. After t ∼1000 days, the spectrum is ﬂattening. The data used for the ﬁts come from K. Weiler (private communication), except for the last data point which is from . 3 Determination of the Shell Width The thickness of the shell has been found to be 30±10 %  (based on ﬁts on the images) and 25±3 %  (based on ﬁts in the uv plane, taking into account the central absorption) of its outer radius.
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