Fig. 8.
Comparison of the spectral parameters of the XDINSs (from Yoneyama et al. 2019) and PSR J0726–2612 (red cross) obtained with two blackbodies and a Gaussian absorption line model (G2BB). Upper panel: blackbody radii (black: cold; green: hot) for the XDINSs and for PSR J0726–2612 (red cross). Lower panel: line width vs. line centroid energy (black dots are for XDINSs and the red cross for PSR J0726–2612).
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