This book presents a brief compilation of results from nearly a
century of research on the globular star clusters in the Andromeda
Galaxy (M31). It explores the techniques and limitations of the
observations, the successes and challenges of the models, and the
paradigm for the formation of M31 that has gradually emerged. These
results will eventually be superseded by new data, better analysis
techniques, and more complex models. However, the emphasis of this
book is on the techniques, thought processes, and connections with
other studies.
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