A star-by-star correspondence between X-ray activity and rotation in the young open cluster NGC 2516 with eROSITA

Open Access

Fig. 2

Example of an eROSITA X-ray spectrum, namely of the cluster member ID 5. The spectrum is fitted with a two-component APEC model (solid line) with respective temperatures of k_BT₁ = 0.68 keV (dotted line) and k_BT₂ = 1.24 keV (dashed line). The lower panel shows the normalised residuals.

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