SUMMARY
A quasar is the luminous output of a supermassive black hole, typically millions to billions of times the mass of the Sun, surrounded by an accretion disk of gas. As matter falls into the black hole, it accelerates and emits immense radiation, making quasars visible across vast distances. When a quasar exhausts its fuel, it transitions into a "quiet" black hole, similar to the one at the center of the Milky Way. The discussion clarifies misconceptions about quasars and their relationship to galaxy formation, emphasizing that supermassive black holes are integral to the initial formation of galaxies.
PREREQUISITES
- Understanding of supermassive black holes
- Knowledge of accretion disks and their role in radiation emission
- Familiarity with the concept of galaxy formation
- Basic grasp of astrophysical phenomena related to black holes and quasars
NEXT STEPS
- Research the properties and behaviors of accretion disks around black holes
- Study the M-sigma relation and its implications for galaxy evolution
- Explore the lifecycle of quasars and their impact on surrounding galaxies
- Investigate the mechanisms of radiation emission from black holes
USEFUL FOR
Astronomers, astrophysicists, and students interested in black hole physics, galaxy formation, and the dynamics of quasars will benefit from this discussion.