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Fig. 2
M• − σ, M• − Mtot, and M• − Ltot relations of IMBHs and SMBHs in comparison. The slope of the best fit to the GCs (green line) is a factor of two shallower than the slope for the SMBHs in galaxies (blue line) for M• − σ, but very similar for the remaining two correlations.
This figure is made of several images, please see below:
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