Star Clusters in M31: Stellar Populations and Mass Loss

Details Star Clusters in M31: Stellar Populations and Mass Loss Star Clusters in M31: Stellar Populations and Mass Loss

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sptz.prop40568b&link_type=abstract

Spitzer Proposal ID #40568

Physics

Scientific paper

We propose an imaging study of massive star clusters in M31 using archival Spitzer imaging with IRAC and MIPS. We have two distinct goals: (1) Estimate cluster ages, metallicities, and reddenings through panchromatic FUV to mid-IR imaging, and (2) Assess the production rate and lifetime of dust in the intracluster medium (ICM) as a function of cluster properties. Our results will give important constraints on the star formation history of M31 and on mass loss in stellar clusters.

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