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Article Contents
- ABSTRACT
- 1.1.INTRODUCTORY REMARKS
- 1.2.CALIBRATION OF STAR FORMATION RATE
INDICATORS ACROSS THE WAVELENGTH SPECTRUM
- 1.2.1.General
characteristics
- 1.2.2.A word about the stellar
initial mass function and stochastic sampling
- 1.3.THE NATURE OF `DIFFUSE' LIGHT
IN GALAXIES
- 1.4.DUST ATTENUATION OF THE
STELLAR LIGHT
- 1.4.1.General properties
- 1.4.2.Application to
galaxies
- 1.5.LESSONS LEARNED
- 1.5.1.Global SFR indicators
- 1.5.2.Local SFR indicators
- REFERENCES