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

Authors

391

  1. CC
    C. Chiappini

    Leibniz Institute for Astrophysics Potsdam, Germany

    8 publications · 937 citations

    8

    h-index

  2. PF
    P. François

    Galaxies, Etoiles, Physique et Instrumentation, France

    5 publications · 394 citations

    5

    h-index

  3. DS
    David S. Aguado

    Instituto de Astrofísica de Canarias, Spain

    5 publications · 247 citations

    5

    h-index

  4. KA
    Kim A. Venn

    University of Victoria, Canada

    4 publications · 140 citations

    4

    h-index

  5. PJ
    P. Jablonka

    École Polytechnique Fédérale de Lausanne, Switzerland

    4 publications · 361 citations

    4

    h-index

1–5 of 391

Venues

  1. Monthly Notices of the Royal Astronomical Society

    21 publications · 1.5K citations

    19

    h-index

  2. Astronomy and Astrophysics

    15 publications · 1.5K citations

    15

    h-index

  3. The Astrophysical Journal

    ApJ · 8 publications · 336 citations

    8

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 392 citations

    4

    h-index

  5. arXiv (Cornell University)

    Repository · 3 publications · 180 citations

    3

    h-index

1–5