Inside-out Growth

Inside-Out Growth is a theoretical model of galaxy evolution in which a galaxy's central regions form and evolve prior to its outer disk, distinguishing it from alternative models by emphasizing earlier star formation and mass assembly in the interior compared to the outskirts.

90

Publications

7.8K

Citations

484

Authors

229

Institutions

Publications per year

2017–2026

32

Authors

484

  1. SF
    S. F. Sánchez

    Universidad Nacional Autónoma de México, Mexico

    8 publications · 1.4K citations

    8

    h-index

  2. CB
    Chris B. Brook

    Universidad Autónoma de Madrid, Spain

    4 publications · 363 citations

    4

    h-index

  3. DM
    D. Mast

    Instituto de Astrofísica de Andalucía, Spain

    4 publications · 919 citations

    4

    h-index

  4. RM
    R. M. González Delgado

    Instituto de Astrofísica de Andalucía, Spain

    4 publications · 816 citations

    4

    h-index

  5. BH
    B. Husemann

    Max Planck Institute for Astronomy, Germany

    4 publications · 919 citations

    4

    h-index

1–5 of 484

Venues

  1. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.7K citations

    23

    h-index

  2. The Astrophysical Journal

    ApJ · 22 publications · 2.2K citations

    19

    h-index

  3. Astronomy and Astrophysics

    14 publications · 1.7K citations

    14

    h-index

  4. The Astrophysical Journal Letters

    4 publications · 635 citations

    4

    h-index

  5. Nature Astronomy

    2 publications · 60 citations

    2

    h-index

1–5