gravitational collapse model
C325
concept
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.
All labels observed (2)
| Label | Occurrences |
|---|---|
| astrophysical concept | 11 |
| gravitational collapse model canonical | 2 |
Instances (13)
| Instance | Via concept surface |
|---|---|
|
Salpeter
surface form:
Salpeter initial mass function
|
astrophysical concept |
| Salpeter initial mass function | astrophysical concept |
| Bonnor–Ebert mass | astrophysical concept |
| Oppenheimer–Snyder model | — |
|
Dan Alderson
surface form:
Alderson disk
|
astrophysical concept |
| LTB metric | — |
| Roche ellipsoid | astrophysical concept |
| Population II | astrophysical concept |
| Oppenheimer–Volkoff limit | astrophysical concept |
| Jeans mass | astrophysical concept |
| Eddington limit | astrophysical concept |
| Gamow peak | astrophysical concept |
| Chandrasekhar limit | astrophysical concept |