Spatially resolved X-ray spectroscopy and modeling of the nonthermal emission of the pulsar wind nebula in G0.9+0.1

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Fig. 2

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Smoothed XMM-Newton count map merged from the MOS and pn data of the 2000 and 2003 observations (see Table 1) in the energy range 3−10 keV. The annuli are encompassed by dashed cyan lines (properties listed in Table 3).

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