Multiple Populations in Integrated Light Spectroscopy of Intermediate Age Clusters
Nate Bastian, Christopher Usher, Sebastian Kamann, Carmela Lardo,, S{\o}ren S. Larsen, Ivan Cabrera-Ziri, William Chantereau, Silvia Martocchia,, Maurizio Salaris, Ricardo P. Schiavon, Randa Asa'd, and Michael Hilker

TL;DR
This study investigates the presence of multiple stellar populations in intermediate-age clusters using integrated light spectroscopy, finding evidence of such populations in a massive cluster, which supports the idea that young massive clusters are similar to ancient globular clusters.
Contribution
It demonstrates the feasibility of detecting multiple populations in integrated light spectra of intermediate-age clusters, especially in very massive clusters, expanding the methods for studying stellar populations.
Findings
No Na spreads in NGC 1978 consistent with resolved star studies
Clear evidence of multiple populations in G114
Supports similarity between young massive and ancient globular clusters
Abstract
The presence of star-to-star light-element abundance variations (a.k.a. multiple populations, MPs) appears to be ubiquitous within old and massive clusters in the Milky Way and all studied nearby galaxies. Most previous studies have focussed on resolved images or spectroscopy of individual stars, although there has been significant effort in the past few years to look for multiple population signatures in integrated light spectroscopy. If proven feasible, integrated light studies offer a potential way to vastly open parameter space, as clusters out to tens of Mpc can be studied. We use the NaD lines in the integrated spectra of two clusters with similar ages ( Gyr) but very different masses, NGC 1978 ( Msun) in the LMC and G114 ( Msun) in NGC 1316. For NGC 1978, our findings agree with resolved studies of individual stars which did not find evidence…
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