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De re metallica: the cosmic chemical evolution of galaxies

Open access
Maiolino, R., Mannucci, F.·2019·The Astronomy and Astrophysics Review

Abstract

The evolution of the content of heavy elements in galaxies, the relative chemical abundances, their spatial distribution, and how these scale with various galactic properties, provide unique information on the galactic evolutionary processes across the cosmic epochs.In recent years major progress has been made in constraining the chemical evolution of galaxies and inferring key information relevant to our understanding of the main mechanisms involved in galaxy evolution.In this review we provide an overview of these various areas.After an overview of the methods used to constrain the chemical enrichment in galaxies and their environment, we discuss the observed scaling relations between metallicity and galaxy properties, the observed relative chemical abundances, how the chemical elements are distributed within galaxies, and how these properties evolve across the cosmic epochs.We discuss how the various observational findings compare with the predictions from theoretical models and numerical cosmological simulations.Finally, we briefly discuss the open problems and the prospects for major progress in this field in the nearby future.

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Metadata

Authors
Maiolino, R., & Mannucci, F.
Venue
The Astronomy and Astrophysics Review
Published
2019-02-04
Volume
27
Issue
1
ISSN
  • 0935-4956 (ISSN-L)
  • 1432-0754
OpenAlex
W2901112184
Cited by
697
References
12
FWCI
37.74
Type
journal article
Language
en
Open access
hybrid

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CoChat. (2026). Citation check: De re metallica: the cosmic chemical evolution of galaxies. https://app.cochat.ai/papers/10.1007/s00159-018-0112-2
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Maiolino, R., & Mannucci, F. (2019). De re metallica: the cosmic chemical evolution of galaxies. The Astronomy and Astrophysics Review. https://doi.org/10.1007/s00159-018-0112-2

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