A correlation between central supermassive black holes and the globular cluster systems of early-type galaxies

@article{Burkert2010ACB,
  title={A correlation between central supermassive black holes and the globular cluster systems of early-type galaxies},
  author={Andreas Burkert and Scott Tremaine},
  journal={The Astrophysical Journal},
  year={2010},
  volume={720},
  pages={516-521}
}
Elliptical, lenticular, and early-type spiral galaxies show a remarkably tight power-law correlation between the mass M • of their central supermassive black hole (SMBH) and the number N GC of globular clusters (GCs): M • = m •/ × N 1.08±0.04 GC with m •/ = 1.7 × 105 M ☉. Thus, to a good approximation the SMBH mass is the same as the total mass of the GCs. Based on a limited sample of 13 galaxies, this relation appears to be a better predictor of SMBH mass (rms scatter 0.2 dex) than the M… 

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