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Table 2

Best-fit parameters derived from the X-ray spectral analysis of three representative subregions and the entire remnant.

Region A region B region C region Entire remnant
Area (106 arcs2) 7.13 4.23 5.23 104.36

Surf_bri (10−3 c arcs−2) 1.92 3.36 2.25 1.66

Model vapec+vapec

kT (keV)
NH(1022cm−2)
O
Ne
Mg
Fe

χ2/d.o.f. 1.03 1.01 1.19

Model vnei+vnei

kT (keV)
NH(1022 cm−2)
O
Ne
Mg
Ionization time (1010 s cm−3)

χ2/d.o.f. 0.88 1.06 1.26

Model vpshock+vpshock

kT (keV)
NH(1022 cm−2)
O
Ne
Mg
Ionization time (1011s cm−3)

χ2/d.o.f. 0.87 1.06 1.16 1.19

Model vnei+vapec

kT (keV)
NH(1022cm−2)
O
Ne
Mg
Ionization time (1011 s cm−3) 2.43 NaN

χ2/d.o.f. 1.03 0.99

Notes. The best-fit parameters are reported with 1σ errors. The three subregions (defined via the Voronoi analysis process) have been selected as representatives to exhibit best the spectral variation detected across the remnant. Where not defined, elemental abundances were set to solar values.

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