The <i>Gaia</i> -ESO survey: Open clusters as tracers of galactic chemical evolution

Aims . We investigate the formation and evolutionary trajectory of the Milky Way’s inner and outer galactic regions using stars from open clusters in the Gaia -ESO OC survey. Methods . Using numerical simulations from Chempy, we leveraged Markov chain Monte Carlo sampling techniques to derive galactic evolutionary parameters for each open cluster by fitting measured abundances of elements C, N, O, Mg, Si, Ca, Ti, Fe, Mn, Zn, Y, and Ba. Results . We find differing evolutionary histories between the inner and outer regions of the Milky Way that align with variations in the slope of the initial mass function, the rate of Type Ia supernovae, and the galactic metallicity gradient traced by open clusters. Conclusions . Our results support established galactic formation and evolutionary theories, highlighting that the inner Galaxy had a short and intense early star formation epoch followed by reduced activity. In contrast, the outer Galaxy maintained a more sustained star formation history.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-11-03
DOI
https://doi.org/10.1051/0004-6361/202556408
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

The Gaia -ESO survey: Open clusters as tracers of galactic chemical evolution

Sarah L. Martell, G. Tautvaišienė, G. Gilmore, F. Jiménez-Esteban et al.
Astronomy and Astrophysics
Stellar, planetary, and galactic studies
article

The Gaia -ESO survey: Open clusters as tracers of galactic chemical evolution

Sarah L. Martell, G. Tautvaišienė, G. Gilmore, F. Jiménez-Esteban, L. Magrini, F. Damiani, E. Stonkuté, A. Drazdauskas, S. Randich, A. Bragaglia, T. Bensby, C. C. Worley, Keith Boucher
article en

Abstract

Aims . We investigate the formation and evolutionary trajectory of the Milky Way’s inner and outer galactic regions using stars from open clusters in the Gaia -ESO OC survey. Methods . Using numerical simulations from Chempy, we leveraged Markov chain Monte Carlo sampling techniques to derive galactic evolutionary parameters for each open cluster by fitting measured abundances of elements C, N, O, Mg, Si, Ca, Ti, Fe, Mn, Zn, Y, and Ba. Results . We find differing evolutionary histories between the inner and outer regions of the Milky Way that align with variations in the slope of the initial mass function, the rate of Type Ia supernovae, and the galactic metallicity gradient traced by open clusters. Conclusions . Our results support established galactic formation and evolutionary theories, highlighting that the inner Galaxy had a short and intense early star formation epoch followed by reduced activity. In contrast, the outer Galaxy maintained a more sustained star formation history.

Astronomy and AstrophysicsVol. 705
University of Canterbury (NZ), Lund University (SE), University of Cambridge (GB), Arcetri Astrophysical Observatory (IT), UNSW Sydney (AU), Institute of Astronomy (RU), Institute of Theoretical Physics (CN), Osservatorio Astronomico di Palermo (IT), Centro de Astrobiología (ES), National Institute for Astrophysics (IT)
Openalex Percentile: Top 78%
Stellar, planetary, and galactic studies
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