Fig. 9.
Brightest cluster MV–SFR relation for different galaxy samples. The NGC 5291S data point with the lowest SFR shows the value for S* only. The black line shows the fit of the Larsen (2002) sample. The dashed green line shows the maximum MV expected for a given SFR if all the star formation occurs in clusters with a 
power law (Bastian 2008).
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