The XMM-Newton and NuSTAR view of IRASF11119+3257 - I. Detection of multiple ultra fast outflow components and a very cold corona

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Fig. 8.

Confidence contour levels of the DISK-WIND parameters f_v vs. μ (left) and ${\dot{M}}_{w}$ $\mathcal{\dot M}_{\mathrm{w}}$ vs. ℒ_X (right), see subsection 6.2 for their definitions. The ${\dot{M}}_{w}$ $\mathcal{\dot M}_{\mathrm{w}}$ vs. ℒ_X contours are obtained by fixing f_v and μ to their closest grid points (marked with the magenta cross) to avoid interpolation issues.

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