Fig. 10.
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Evolutionary tracks of the SNR #22 in the shape phase-space for the various explosion models. Uncertainties due to the choice of Zej, thr are shown as shaded regions. In different parts of the phase space the SNRs are either spherical (S), oblate-spheroidal (OS), prolate (P), or oblate (O). The SNR starts out as a perfect sphere and becomes increasingly prolate over time. The ratio of the two minor axes remains close to one and never falls below 2/3. In the model N10 the SNR remains spherical for longer compared to N1. Similarly the consecutive SN explosions in the model N1×10 restore spherical symmetry.
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