Nuclear star clusters around supermassive black holes develop a collision-regulated density profile n(r) ∝ r^-5/4, independent of whether scattering or gravitational waves drive the orbits.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.GA 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Dynamics in Nuclear Stellar Clusters: The Impact of Collisions and Disrupted Binaries
Nuclear star clusters around supermassive black holes develop a collision-regulated density profile n(r) ∝ r^-5/4, independent of whether scattering or gravitational waves drive the orbits.