Fig. 15
MBH–Mbulge relation for 35 early-type galaxies in the local Universe (empty diamonds) and BR 1202 S (red filled circle; the empty filled circle also considers the contribution from the dispersion-supported mass). The black line represents the best-fitting relation estimated by McConnell & Ma (2013): log (MBH/M⊙) = 8.46 + 1.05log (Mbulge/1011M⊙).
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