Disentangling the X-ray variability in the Lyman continuum emitter Haro 11

Open Access

Fig. 7.

Simulated spectra of the XMM-Newton EPIC-pn (91 ks) and Chandra ACIS-S X1 and X2 sources (127 ks) using the model parameters listed in Table 3, including the emission lines suggested by our PCA, as labeled in Fig. 5.

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