Attributing the point symmetric structure of core-collapse supernova remnant N132D to the jittering jets explosion mechanism
Noam Soker (Technion, Israel)

TL;DR
This paper identifies a point-symmetric structure in supernova remnant N132D, supporting the jittering jets explosion mechanism (JJEM) as the primary cause of core-collapse supernovae, contrasting with neutrino-driven models.
Contribution
It provides observational evidence of point-symmetry in N132D consistent with JJEM, strengthening its role as the main explosion mechanism for CCSNe.
Findings
Point-symmetric morphology correlates with explosion mechanism.
Two perpendicular jet pairs shape the remnant structure.
Supports JJEM over neutrino-driven models.
Abstract
I identified a point-symmetric morphology in the core-collapse supernova (CCSN) remnant (CCSNR) N132D, composed of two symmetry axes: the short symmetry axis extending from the northwest ear and through the center of the iron-rich emission on the other side, and the second along the long dimension of N132D and coincides with the extension of the central oxygen-rich gas to the northeast. Namely, the point-symmetry of the outer zones of CCSNR N132D correlates with that of the oxygen-rich gas near the center. The surrounding gas cannot shape the inner oxygen-rich material, implying that the point-symmetric morphology is a property of the explosion mechanism, as predicted by the jittering jets explosion mechanism (JJEM). The oxygen-rich material is known to be in a torus. According to the JJEM, an energetic pair of opposite jets, more or less perpendicular to the plane of the torus, has…
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