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Constraining the Circumstellar Medium Structure and Progenitor Mass-Loss History of Interacting Supernovae Through 3D Hydrodynamic Modeling: The Case of SN 2014C

Salvatore Orlando et al 2024 ApJ 977 118 Three-dimensional hydrodynamical modeling of the supernova SN 2014C suggests that the progenitor star lost 2.5 solar masses of material during the period from…

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Kerry Hensley1y agoen

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