Observational analysis reveals black holes influence characteristics in globular clusters, suggesting new astrophysics insights.
In this paper, a sample of globular clusters (GCs) is created for which the masses of black holes in their centers are known from observations. The dependence of the main characteristics of GCs on the mass of black holes is studied.Based on observational data on the surface density of GCs, the degree of concentration of stars to their center is determined. The obtained degree of concentration is used as an indicator of the presence of black holes.
No takes yet. Share an insight, caveat, or question.
S. N. Nuritdinov (2025) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: