The main jet axis of the W49B supernova remnant
Noam Soker, Dmitry Shishkin

TL;DR
This paper identifies a main jet axis in the supernova remnant W49B through morphological analysis, supporting the idea that jets played a significant role in its explosion, likely indicating a core-collapse supernova origin.
Contribution
It presents the first identification of a main jet axis and circum-jet rings in W49B, providing evidence for jet-driven explosion mechanisms in this supernova remnant.
Findings
Identification of a main jet axis connecting opposite ears.
Detection of circum-jet ring signatures around the axis.
Evidence supporting a core-collapse supernova origin.
Abstract
We identify an axis connecting two opposite `ears' in the supernova remnant W49B and morphological signatures of three arcs around this axis that we claim are sections of full circum-jet rings. Based on recent identifications of morphological signatures of jets in core-collapse supernovae (CCSNe), including ejecta-rich axes, we reexamine images of W49B and identify a heavy element-rich protrusion (ear) as a jet-inflated structure. We identify the opposite ear and a clump at its tip as the signature of the opposite jets. The line connecting the two clumps at the tips of the two opposite ears forms the main jet axis of W49B. We compare the three arcs around the main jet axis in W49B to the circum-jet rings of the jets in the Cygnus A galaxy and deduce that these arcs are sections of full circum-jet rings in W49B. In W49B, the jets are long gone, as in some planetary nebulae with…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Gamma-ray bursts and supernovae
