Fig. 8
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Mean MLR vs median period for our sample (grey circles). Sources with vinf>17 km s−1 are coloured according to their SIMBAD object type. The fit from De Beck et al. (2010) (dashed curve) reproduces the increasing trend in our data well. The saturation MLR from our broken-power law fit (Equation (4), solid line) is also shown for comparison.
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