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Raffaella Margutti edited figures/mdotplot/caption.tex
over 8 years ago
Commit id: 1f2db57fc23e4722b3baa48aee50b05176fd69d6
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The density profile
around a nearby Ib SN as probed by recent radio observations (black solid line) violates the expectations from the standard theory of line driven winds (orange line), requires a different physical explanation and motivates a deep and rigorous search for density enhancements in the environment of core-collapse SNe.
