X-ray spectra of young Type I supernova remnants - Exploded white dwarfs?

It is argued that the X-ray spectra of young Type I supernova remnants can be understood consistently in terms of thermal emission mainly from a reverse shock into initially uniform density ejecta. The inferred mass of ejecta is then consistent with 1.4 solar mass in SN 1006, Tycho, and Kepler. A substantial mass of iron, perhaps 0.8 solar mass, may be present provided that the ejecta are chemically inhomogeneous, with iron confined to inner layers of ejecta. The marked difference between the X-ray spectra of SN 1006 and Tycho is explained by the lower interstellar density around SN 1006.