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Properties of Stellar Clusters and their Relation to Molecular Gas in the Andromeda Galaxy
The apparent age and mass of a stellar cluster can be strongly affected by stochastic sampling of the stellar initial mass function, when inferred from the integrated color of low mass clusters ($\lesssim$ $10^4$ $M_{\odot}$). I use simulated star clusters to show that these effects are minimized when the brightest, rapidly ...