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Ultrafast outflows in ultraluminous X-ray sources

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Fig. 1 Soft X-ray residuals to continuum models for 6 ULXs. The objects are: (a) NGC 1313 1, (b) Ho IX X-1, (c) Ho II X-X-1, (d) NGC 55 ULX-X-1, (e) NGC 6946 X-X-1, and (f) NGC 5408 X-1
Fig. 2 Absorption strength from the spectral fits plotted against spectral hardness (with 1σ error bars)
Fig. 3 XMM-Newton/RGS high-resolution grating spectra of NGC 1313 X-1 and NGC 5408 X-1 (top) with overlaid a model of thermal collisionally-ionized emission and a relativistically (v ∼ 0.2c blueshifted photoionized absorption
Fig. 4 Detection of Fe K blueshifted absorption (6.70 keV lab energy) in the combined XMM-Newton EPIC CCD and NuSTAR FPMA/B CdZnTe spectra

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