Kavli Affiliate: Lars Bildsten | First 5 Authors: Kathlynn Simotas, Kathlynn Simotas, , , | Summary: Thermonuclear supernovae (SNe) are the result of the nuclear transformation of carbon/oxygen (C/O) white dwarfs (WDs) to the radioactive element $^56mathrmNi$ and intermediate mass elements (IMEs) like Ca, Ar, etc. Most progenitor scenarios involve a companion star which donates […]
Continue.. Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles