A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2017; you can also visit the original URL.
The file type is
The relationship between Type Ia supernovae and the thermal X-ray emission from their young supernova remnants is explored using one dimensional hydrodynamics and self- consistent ionization and electron heating calculations coupled to a spectral code. The interaction with the ambient medium is simulated for a grid of supernova explosion models which includes all the physical mechanisms currently under debate. The differences in density profile and chemical composition of the ejecta for eachdoi:10.5281/zenodo.47938 fatcat:r7v6vw6hijghlolnoagh3ocln4