gravitational collapse model

A gravitational collapse model is a theoretical framework that describes how matter in astrophysical systems contracts under its own gravity, potentially leading to the formation of dense objects such as stars, black holes, or compact stellar remnants.

Observed surface forms (1)

• astrophysical concept ×4

Instances (5)

• Oppenheimer–Snyder model
• Oppenheimer–Volkoff limit via concept surface "astrophysical concept"
• Jeans mass via concept surface "astrophysical concept"
• Eddington limit via concept surface "astrophysical concept"
• Chandrasekhar limit via concept surface "astrophysical concept"