Chemo-dynamical Evolution
Chemo-Dynamical Evolution is a theoretical framework in astrophysics that integrates the chemical enrichment and dynamical processes of stars and interstellar matter to model the co-evolution of the Galactic Disk and Galactic Halo within a single, self-consistent narrative.
64
Publications
4.5K
Citations
391
Authors
208
Institutions
Publications per year
2017–2026
24
Parents
64
Chemodynamical evolution of the Milky Way disk
Astronomy and Astrophysics · 2013 · 441 citations · Full text
Natural Sciences, Astronomy, Physics +15
Chemodynamical evolution of the Milky Way disk
Ivan Minchev, C. Chiappini, Marie Martig · Astronomy and Astrophysics · 2014 · 249 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 64
391
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1–5 of 391
208

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
16 h-index
83 publications
10.2K citations

Centre National de la Recherche Scientifique
Paris, France
16 h-index
34 publications
2K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
10 h-index
10 publications
648 citations
University of Cambridge
Cambridge, United Kingdom
9 h-index
33 publications
3.5K citations
Heidelberg University
Heidelberg, Germany
8 h-index
16 publications
854 citations
Institute of Astronomy
Moscow, Russia
8 h-index
15 publications
744 citations
Galaxies, Etoiles, Physique et Instrumentation
Meudon, France
8 h-index
25 publications
2.5K citations
Osservatorio Astronomico di Padova
Padua, Italy
7 h-index
16 publications
1.6K citations
1–8 of 208
21 publications · 1.5K citations
19
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15 publications · 1.5K citations
15
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ApJ · 8 publications · 336 citations
8
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Repository · 4 publications · 392 citations
4
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Repository · 3 publications · 180 citations
3
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1–5