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Fig. 2
LX − R distribution for ALL-XRBs (top), NS-XRBs (middle), and BH-XRBs (bottom). Sources from M 82, NGC 1569, and NGC 5253 in Kaaret et al. (2004, see their Fig. 3 samples are also shown as diamonds, triangles and squares, respectively for comparison. From left to right are models M1, M2, BAC, and M3.
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