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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 1.1.Context
- 1.2.Scope of this review
- 2.BACKGROUND AND CHALLENGES
- 2.1.Overview and history
- 2.2.IMF definitions and
terminology
- 2.3.Conventions and language
usage
- 2.3.1.Sign conventions
- 2.3.2.IMF naming
conventions
- 2.3.3.Parameter ranges
- 2.3.4.IMF shape
descriptions
- 2.3.5.Other issues
- 2.4.The confusion wrought through
"universality"
- 3.IMF MEASUREMENT APPROACHES: STELLAR
TECHNIQUES
- 3.1.Resolved star counts and
luminosity functions
- 3.2.Stellar clusters
- 3.3.Chemical abundance
measurements
- 3.4.Population III stars
- 3.5.Review
- 4.IMF MEASUREMENT APPROACHES: NEUTRAL
AND MOLECULAR GAS AND DUST
- 5.IMF MEASUREMENT APPROACHES:
INTEGRATED GALAXY TECHNIQUES
- 5.1.Background
- 5.2.Star forming galaxies
- 5.3.Passive galaxies
- 5.4.Summary and limitations
- 5.5.Linking galaxies to their
constituents
6.IMF MEASUREMENT APPROACHES: COSMIC
CENSUS TECHNIQUES
7.IMF MEASUREMENT APPROACHES:
SIMULATIONS AND MODELS
7.1.Simulating star
formation
7.2.Simulating galaxy
evolution
8.A CONSISTENT APPROACH
8.1.IMF constructs
8.2.Linking mass functions between
different spatial scales
8.3.Derived quantities
8.4.Implementation
8.5.A broader context
9.DISCUSSION
9.1.What do the observations
really tell us?
9.2.Unifying our understanding
of the IMF
9.3.Is the IMF universal?
9.4.Future work
10.CONCLUSIONS
REFERENCES