astro-ph.HE
Constraining the CSM structure and progenitor mass-loss history of interacting supernovae through 3D hydrodynamic modeling: The case of SN 2014C
S. Orlando E. Greco R. Hirai T. Matsuoka M. Miceli S. Nagataki M. Ono K. -J. Chen D. Milisavljevic D. Patnaude F. Bocchino N. Elias-Rosa