📝 SummarXiv

Abstract

I find that the dust morphologies in some core-collapse supernova (CCSN) remnants (CCSNRs) possess jet-shaped morphologies, and propose that the properties of the jets that explode the CCSNe and their interaction with the core and envelope (if it exists) are among the factors that determine the amount of dust formed and its morphology. I find that some of the dust-rich structures in the CCSNRs Cassiopeia A and the Crab Nebula are distributed in point-symmetric morphologies, and that the dust in SN 1987A follows the bipolar morphology of the inner ejecta. Earlier studies attributed these morphologies in these CCSNRs to shaping by jets in the framework of the jittering jets explosion mechanism (JJEM). These dust morphologies suggest, in the framework of the JJEM, that exploding jets enhance dust formation in CCSNRs. This study adds to the variety of processes that CCSN exploding jets are involved in and to the establishment of the JJEM as the explosion mechanism of CCSNe.