Recent evolution of the star cluster population in the Andromeda’s disk

Abstract

The most accurate parameters of star clusters are determined by analyzing colour-magnitude diagrams (CMDs) constructed from their member stars. The recent study applying this method to the analysis of the Panchromatic Hubble Andromeda Treasury (PHAT) survey star clusters includes objects up to ages of 300 Myr. In this study, we aim to extend a sample of star clusters with parameters determined based on CMDs of individual stars to older ages, up to ~700 Myr. We have developed an isochrone fitting procedure for CMDs of resolved and semi-resolved clusters to determine their parameters. The Bayesian approach is employed in determining star cluster ages and interstellar extinctions. We determined ages and extinctions for a sample of 854 star clusters from the M31 PHAT survey. We found that the star formation rate in the M31 galaxy was rather constant during the last ~130 Myr; however, a strong cluster formation episode occurred ~220 Myr ago, and can be attributed to the predicted passage of the M32 galaxy through the Andromeda’s disk.