Nickel Bubble Expansion in Type Ia Supernovae: Adiabatic Solutions
classification
🌌 astro-ph
keywords
typebubblenickelsolutionssupernovaeadiabaticapplicationcomparison
read the original abstract
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.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.