Fig. 9.

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Observations of GX 339-4 in the ṁin−rJ plane (top), bolometric luminosity (Lbol) computed from our model (middle), and 1−10 keV luminosity (L1−10 keV) as function of ṁin (bottom). In all panels the color is the ratio of bolometric radiated power to the power advected (see color bar). The different lines are shown in orange to illustrate different regimes: solid when , and dotted and dashed for the two different regimes when L ∝ ṁin.
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