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Numerical calculations are presented for supernova ejecta with initially constant total energy E0 expanding into an interstellar medium of uniform density n0, assuming perfect spherical symmetry. Scaling laws are presented for changes in E01n0 with constant E0n02. Results are given for the time development of various quantities, including the emitted X-ray spectrum, for three different values of E0n02. Subject headings: supernova remnants - X-rays
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Mansfield et al. (1974) studied this question.
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