STScI Preprint #1352
This review addresses properties and unresolved issues of stellar systems whose ages are young in comparison with a Hubble time. In most cases, the energy production in such systems is determined by massive, short-lived stars. These stars track the most recent star-formation history in stellar clusters and galaxies. Due to their intrinsic brightness, even relatively few such stars are observable at cosmological distances. I discuss the current state of our understanding of massive stars and how uncertainties affect the interpretation of young stellar systems and galaxies.
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218