2012/08/22 by F. Taddia, M. Stritzinger, M. D. Stritzinger +25 · 5 citations
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Emission spectrum #Extinction (optical mineralogy) #Gamma-ray bursts and supernovae #Light curve #Optics #Physics #Spectral line #Spectroscopy #Supernova #astro-ph.HE #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/201220105
8 pages, 4 figures, minor changes to match the published version
openalex publication_date 2012/08/22 · arxiv created 2012/09/15 · arxiv updated 2015/06/11 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/06
Aims. We provide additional observational evidence that some Type Ia supernovae (SNe Ia) show signatures of circumstellar interaction (CSI) with hydrogen-rich material.