Intermediate Black Holes

Intermediate black holes are a class of black holes that are larger than stellar black holes, but smaller than supermassive black holes. They typically have masses ranging from hundreds to thousands of times the mass of the sun.

Formation

Intermediate black holes are thought to form through the following processes:

• Merger of smaller black holes
• Direct collapse of massive gas clouds
• Runaway collisions of stars in dense star clusters

Characteristics

Intermediate black holes exhibit the following characteristics:

• Strong gravitational pull
• Ability to devour nearby stars and gas clouds
• Possibly located in the centers of globular clusters or dwarf galaxies

Study Guide

To study intermediate black holes, you should focus on the following key areas:

1. Formation mechanisms
2. Mass range and physical characteristics
3. Observational evidence and detection methods
4. Role in the evolution of galaxies

Additionally, it's important to understand the differences between intermediate black holes, stellar black holes, and supermassive black holes, as well as their implications for our understanding of the universe.

Be sure to review relevant astronomical observations, theoretical models, and current research in the field of black hole astrophysics.

Good luck with your studies!