Asymmetries in core-collapse supernovae from maps of radioactive 44Ti in Cassiopeia A
(1st sentence)
Asymmetry is required by most numerical simulations of stellar core-collapse explosions, but the form it takes differs significantly among models.
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(Last sentence)
As neither the spherically symmetric nor the strongly asymmetric explosion reproduces all of the observed properties of the 44Ti spatial distribution, the progenitor of the Cas A remnant was most probably between these two extremes: a mildly asymmetric explosion developing low-mode convection.
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