2014年4月14日月曜日

Asymmetries in core-collapse supernovae from maps of radioactive 44Ti in CassiopeiaA




(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 CasA remnant was most probably between these two extremes: a mildly asymmetric explosion developing low-mode convection.

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