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Fig. 22

image

Same as in Fig. 18, but at the age of ≈2000 yr for model W15-2-cw-IIb-HD+dec. The solid white cross marks the ranges of kTe and ne t of the bulk of the ejecta derived from Chandra X-ray observations of the SNR G292 (Bhalerao et al. 2019); the dashed lines mark the extreme values of kTe and ne t inferred for isolated knots in the northwest hemisphere of the remnant.

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