Identifying a point-symmetric morphology in supernova remnant Cassiopeia A: explosion by jittering jets

TL;DR

This paper presents evidence of a point-symmetric morphology in supernova remnant Cassiopeia A, supporting the jittering jets explosion mechanism over traditional neutrino-driven models.

Contribution

It identifies multiple pairs of opposite jets and symmetry axes in Cassiopeia A, providing morphological evidence for the jittering jets explosion mechanism in core-collapse supernovae.

Findings

Seven pairs of opposite morphological features linked to jets

Identification of a point-symmetric wind-rose structure

Morphological features challenge neutrino-driven explosion models

Abstract

We identify a point-symmetric morphology of the supernova remnant (SNR) Cassiopeia A compatible with shaping by at least two, and more likely more than four, pairs of opposite jets, as expected in the jittering jets explosion mechanism (JJEM) of core-collapse supernovae. Using an old Spitzer Telescope infrared map of argon, we identify seven pairs of opposite morphological features that we connect with lines that cross each other at the same point on the plane of the sky. The opposite morphological features include protrusions, clumps, filaments, and funnels in the main SNR shell. In addition to these seven symmetry axes, we find two tentative symmetry axes (lines). These lines form a point-symmetric wind-rose. We place this point-symmetric wind-rose on a new JWST and X-ray images of Cassiopeia A. We find other morphological features and one more symmetry axis that strengthen the identified point-symmetric morphology. Not all symmetry axes correspond to jets; e.g., some clumps are formed by the compression of ejecta between two jet-inflated lobes (bubbles). The robust point-symmetric morphology in the iconic Cassiopeia A SNR strongly supports the JJEM and poses a severe challenge to the neutrino-driven explosion mechanism.