Fig. 6
X-ray spectrum of G29.37+0.1 in the 1.5–8.0 keV energy band. We show the merged Chandra (in black) and XMM-Newton (in red) spectra obtained combining the individual spectra for the different observations, as described in the text. The lines are the best-fit with a) an absorbed power-law model and b) an absorbed bremsstrahlung model.
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