Eduardo Bravo
0000-0003-0894-6450
Universitat Politècnica de Catalunya
2 papers found
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Chandrasekhar and Sub-Chandrasekhar Models for the X-Ray Emission of Type Ia Supernova Remnants. I. Bulk Properties
Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
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