Fig. 2
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Intensity representation of the emission of Vela Jr and its CCO J085201.4-461753 in the 1.1–8 keV band as seen by eROSITA’s TM1–TM7. The colors are linearly distributed so that black corresponds to a pixel intensity value of 0 and white to 3 cts pixel−1. The point source at the southeastern rim of the Vela Jr remnant is the 65 ms pulsar PSR J0855-4644.
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