SUMMARY
Globular clusters maintain their spherical shape and do not collapse due to a combination of gravitational balance and pressure support. Unlike rigid bodies, the stars within these clusters exhibit random rotation parameters, which prevents flattening from centrifugal forces. Key factors include stellar velocity dispersion, mass segregation, tidal effects, and the presence of dark matter, which collectively contribute to the stability of these clusters. Additionally, the high mass-to-light ratio and low levels of gas and dust further inhibit collapse.
PREREQUISITES
- Understanding of gravitational dynamics in astrophysics
- Knowledge of stellar kinematics and velocity dispersion
- Familiarity with concepts of mass segregation and tidal forces
- Basic comprehension of dark matter's role in cosmic structures
NEXT STEPS
- Research the role of dark matter in galaxy formation and stability
- Study stellar dynamics and the effects of velocity dispersion in star clusters
- Explore the concept of mass segregation in globular clusters
- Investigate the impact of tidal forces on the structure of star clusters
USEFUL FOR
Astronomers, astrophysicists, and students studying stellar dynamics and the formation of cosmic structures will benefit from this discussion.