Salpeter initial mass function
E253717
UNEXPLORED
The Salpeter initial mass function is a foundational mathematical description in astrophysics that specifies how many stars of different masses form in a given stellar population, characterized by a power-law distribution favoring low-mass stars.
Referenced by (1)
| Subject (surface form when different) | Predicate |
|---|---|
|
Edwin E. Salpeter
→
|
knownFor |