Multiple Populations in Integrated Light Spectroscopy of Intermediate Age Clusters
| Autor: | Maurizio Salaris, W. Chantereau, S. Martocchia, Ricardo P. Schiavon, Carmela Lardo, Christopher Usher, Michael Hilker, I. Cabrera-Ziri, Sebastian Kamann, Søren S. Larsen, Randa Asa'd, Nate Bastian |
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| Přispěvatelé: | Bastian N., Usher C., Kamann S., Lardo C., Larsen So.S., Cabrera-Ziri I., Chantereau W., Martocchia S., Salaris M., Schiavon R.P., Asa'D R., Hilker M. |
| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
Milky Way
Astronomy Population FOS: Physical sciences Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics 01 natural sciences Spectral line Abundance (ecology) 0103 physical sciences Astrophysics::Solar and Stellar Astrophysics Spectroscopy education 010303 astronomy & astrophysics QC Astrophysics::Galaxy Astrophysics QB Physics education.field_of_study 010308 nuclear & particles physics Astronomy and Astrophysics Astrophysics - Astrophysics of Galaxies Galaxy Stars Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) Globular cluster galaxies: star clusters: general |
| Zdroj: | Monthly Notices of the Royal Astronomical Society: Letters, 489, 1, pp. L80-L85 Monthly Notices of the Royal Astronomical Society: Letters, 489, L80-L85 |
| ISSN: | 1745-3933 |
| Popis: | 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 ($2-3$ Gyr) but very different masses, NGC 1978 ($\sim3\times10^5$ Msun) in the LMC and G114 ($1.7\times10^7$ Msun) in NGC 1316. For NGC 1978, our findings agree with resolved studies of individual stars which did not find evidence for Na spreads. However, for G114, we find clear evidence for the presence of multiple populations. The fact that the same anomalous abundance patterns are found in both the intermediate age and ancient GCs lends further support to the notion that young massive clusters are effectively the same as the ancient globular clusters, only separated in age. MNRAS letters, in press (5 pages + appendix) |
| Databáze: | OpenAIRE |
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