Key points are not available for this paper at this time.
Context. For galaxies hosting supermassive black holes (SMBHs), it has been observed that the mass of the central black hole (M•) tightly correlates with the effective or central velocity dispersion (σ) of the host galaxy. The origin of this M• − σ scaling relation is assumed to lie in the merging history of the galaxies, but many open questions about its origin and the behavior in different mass ranges still need to be addressed.
Lützgendorf et al. (Tue,) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: