A compilation of 115 supernova X-ray light curves and selected spectra concludes that Type Ib/c and low-mass-loss Type IIP supernovae emit non-thermally, while Type IIn supernovae emit thermally, with inferred progenitor mass-loss rates below 10^-5 and above 10^-3 solar masses per year respectively.
Detection of X-rays during the outburst of SN 1980 k
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On the X-ray Emission From Supernovae, and Implications for the Mass-Loss Rates of their Progenitor Stars
A compilation of 115 supernova X-ray light curves and selected spectra concludes that Type Ib/c and low-mass-loss Type IIP supernovae emit non-thermally, while Type IIn supernovae emit thermally, with inferred progenitor mass-loss rates below 10^-5 and above 10^-3 solar masses per year respectively.