One approach to learning about stellar populations is to study them
at three different levels of resolution. First in our own Galaxy;
secondly from nearby galaxies where stars can still be resolved;
and thirdly in remote galaxies in which the stellar population can
only be studied in integrated light. This IAU Symposium covered the
entire range of galaxies in its study of their stellar populations.
Interspersed with theoretical papers, the wealth of observational
results provides an important state-of-the-art presentation of the
progress that has been made in this field.
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