### Initial Mass Function

**(IMF)**
(function describing initial mass of stars)

The **Initial Mass Function** (**IMF**) is an
empirical distribution function
(essentially an unnormalized Probability Density Function)
that describes the distribution of initial masses of stars.
It is typically given as N(m)dm.

- m - mass of a star.
- N(m) - number of stars at that mass.

Edwin Salpeter developed an early IMF in 1955,
the **Salpeter function**:

N(m)dm = C × (m/M_{Sun})^{-2.35}(dm/M_{Sun})

C is a constant reflecting local stellar density.

The IMF can be derived from
the Luminosity Function and the Mass-Luminosity Relation.

Note that the phrase *mass function* is to indicate it
deals with physical masses. The two-word phrase is used in probability
(**Probability Mass Function**) for an incompatible concept:
a function yielding the probability of some discrete random variable
taking on a given value.

(*model,relation,stars,mass,function*)
http://en.wikipedia.org/wiki/Initial_mass_function

http://jila.colorado.edu/~pja/astr3830/lecture06.pdf

**Referenced by:**

Dense Core Mass Function (DCMF)

Power Law

Stellar Population Synthesis Code

Stellar Birth Rate Function

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