Constraining the CSM structure and progenitor mass-loss history of interacting supernovae through 3D hydrodynamic modeling: The case of SN 2014C

Documenti analoghi

• Measuring the initial mass of 44Ti in SN 1987A through the 44Sc emission line
  di: Giuffrida, Roberta, et al.
  Pubblicazione: (2025)
• SN 2024cld: unveiling the complex mass-loss histories of evolved supergiant progenitors to core collapse supernovae
  di: Killestein, T. L., et al.
  Pubblicazione: (2025)
• Origin of holes and rings in the Green Monster of Cassiopeia A: Insights from 3D magnetohydrodynamic simulations
  di: Orlando, S., et al.
  Pubblicazione: (2025)
• Filamentary Ejecta Network in Cassiopeia~A Reveals Fingerprints of the Supernova Explosion Mechanism
  di: Orlando, S., et al.
  Pubblicazione: (2025)
• The impact of effective matter mixing based on three-dimensional hydrodynamical models on the molecule formation in the ejecta of SN 1987A
  di: Ono, Masaomi, et al.
  Pubblicazione: (2023)