Overview of Multiple Star Systems

Multiple stars represent approximately 50 % of the stellar population, and as a result, have implications for the dynamics of young star clusters and associations. This chapter reviews several aspects of multiple star systems, namely the field solar-type multiple population, the field OB star multiple population, and finally the open cluster solar-type multiple population. We discuss each in terms of observed distributions and how these vary depending on their environment. Finally, we close with some thoughts concerning the significance of multiple star systems to the dynamics of young star clusters and associations, specifically how these can be used to further constrain star formation processes and whether these systems can be used as a tracer of identifying the origin of the field population.