Radiative-transfer modeling of supernovae in the nebular-phase. A novel treatment of chemical mixing in spherical symmetry

2020/11/01 by Luc Dessart, D. J. Hillier, D. John Hillier
Mathematics · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Circular symmetry #Classical mechanics #Ejecta #Gamma-ray bursts and supernovae #Geometry #Mathematics #Mixing (physics) #Optics #Phase (matter) #Physics #Quantum mechanics #Radiative transfer #Stellar, planetary, and galactic studies #Supernova #Symmetry (geometry) #astro-ph.HE #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/202039287

published as A&A 643, L13 (2020) · Accepted for publication in A&A Letters

arxiv created 2020/11/05 · openalex publication_date 2020/11/05 · arxiv updated 2020/11/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Accepted for publication in A&A Letters

Citations

• Nucleosynthesis and Clump Formation in a Core-Collapse Supernova
• Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh
• Photometric and spectroscopic evolution of the Type IIP supernova SN 2004et