2007/08/28 by F. Patat, S. Benetti, Stephen Justham +12 · 1 citation
Mathematics · Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Biology #Circumstellar disk #Context (archaeology) #Gamma-ray bursts and supernovae #Geology #Limit (mathematics) #Mathematical analysis #Mathematics #Physics #Progenitor #Progenitor cell #Stars #Stellar, planetary, and galactic studies #Supernova #Type (biology) #astro-ph
paper · pdf · doi:10.1051/0004-6361:20078393
6 pages, 3 figures. Accepted for publication in Astronomy and Astrophysics
arxiv created 2007/08/28 · openalex publication_date 2007/08/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context.The nature of the companion stars in type Ia Supernova (SNe) progenitor systems remains unclear. One possible way to discriminate between different scenarios is the presence (or absence) of circumstellar material, the left overs from the progenitor evolution that may be revealed by their interaction with the SN.