2006/06/19 by Chih‐Yueh Wang, Chih-Yueh Wang, Wang, Chih-Yueh
Engineering · Physics and Astronomy · #Astro and Planetary Science #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Space Satellite Systems and Control #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0606446
ApJ, 2008, accepted, 36 pages
openalex publication_date 2006/06/19 · arxiv created 2008/06/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
This paper presents hydrodynamical and radiation-hydrodynamical simulations of the nickel bubble effect in Type Ia supernovae, comparison of results to self-similar solutions, and application to observations of Type Ia supernova remnants, with a particular emphasis on Tycho's SNR.