- PII
- S30345170S0004629925020036-1
- DOI
- 10.7868/S3034517025020036
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 2
- Pages
- 108-112
- Abstract
- 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.
- Keywords
- центральные черные дыры шаровые скопления параметр концентрации звезд к центру поверхностные плотности скоплений
- Date of publication
- 01.02.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 102
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