2015/11/30 by G. Morlino, P. Blasi · 17 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Fermi Gamma-ray Space Telescope #Gamma-ray bursts and supernovae #Near-Earth supernova #Radiation #Shock (circulatory) #Shock wave #Shock waves in astrophysics #Spectral line #Supernova #astro-ph.HE
paper · pdf · doi:10.1051/0004-6361/201527761
published in Astronomy and Astrophysics 589, A7 (EDP Sciences) · 6 pages, 3 figures. Accepted for publication by A&A
arxiv created 2016/03/07 · openalex publication_date 2016/03/09 · arxiv updated 2016/04/06 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. The presence of neutral hydrogen in the shock proximity changes the structure of the shock and affects the spectra of particles accelerated through the first-order Fermi mechanism. This phenomenon has profound implications for the interpretation of the multifrequency spectra of radiation from supernova remnants.