Shadows of our Former Companions: How the Single-Degenerate Binary Type Ia Supernova Scenario Affects Remnants
High Energy Astrophysical Phenomena
2016-12-14 v1
Abstract
Here we present three-dimensional high resolution simulations of Type Ia supernova in the presence of a non-degenerate companion. We find that the presence of a nearby companion leaves a long-lived hole in the supernova ejecta. In particular, we aim to study the long term evolution of this hole as the supernova ejecta interacts with the surrounding interstellar medium. Using estimates for the x-ray emission, we find that the hole generated by the companion remains for many centuries after the interaction between the ejecta and the interstellar medium. We also show that the hole is discernible over a wide range of viewing angles and companion masses.
Keywords
Cite
@article{arxiv.1609.06319,
title = {Shadows of our Former Companions: How the Single-Degenerate Binary Type Ia Supernova Scenario Affects Remnants},
author = {William J Gray and Cody Raskin and J. Michael Owen},
journal= {arXiv preprint arXiv:1609.06319},
year = {2016}
}
Comments
12 pages, 14 figures, accepted to ApJ