Fig. 3
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Energy-selected eROSITA (TM1-TM7) view of the Vela Jr region. The images are centered on the position of the CCO. Intensity vs. color are distributed according to the ASINH-function. The color vs. cts pixel−1 distribution in each image is depicted. For the 0.7–1.0 keV images a scale of 0–6 cts pixel−1, and for the 1.1–1.3 keV images a scale of 0–2 cts pixel−1 were used. Below ~ 1 keV emission from the Vela SNR dominates. Above ~ 1 keV the nonthermal emission from Vela Jr starts to stand out above the emission from Vela SNR.
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