Fig. 5: Expanded Fermi-LAT TS map.
From: A cosmic-ray loaded nascent outflow driven by a massive star cluster
Same as Fig. 1, with additional information: White plus markers indicate positions of 4FGL-DR4 sources that are part of the fitted ROI model; blue-green × markers of those removed from the model. The dotted circles denote the extension of the disk sources 4FGL J1652.2–4633e and 4FGL J1655.5–4737e. The two green square markers show the position of 4FGL J1648.4–4611 and 4FGL J1650.3–4600 (associated with the pulsars PSR J1648–4611 and PSR J1650–4601, respectively). Shown in red are regions 1, 2, 3, for which separate energy spectra have been derived from Fermi-LAT and H.E.S.S. data (cf. Fig. 7).
