Accretion Histories

Accretion History is a theoretical construct in astrophysics that denotes the chronological sequence and characteristics of mergers and mass incorporations through which a galaxy, particularly its halo, has grown over time by capturing smaller satellite systems and globular clusters.

175

Publications

22.7K

Citations

530

Authors

326

Institutions

Publications per year

2017–2026

58

Authors

530

  1. VB
    Vasily Belokurov

    University of Cambridge, United Kingdom

    6 publications · 777 citations

    6

    h-index

  2. JF
    Julio F. Navarro

    University of Victoria, Canada

    6 publications · 1.8K citations

    6

    h-index

  3. RH
    Risa H. Wechsler

    Kavli Institute for Particle Astrophysics and Cosmology, United States

    6 publications · 4.4K citations

    6

    h-index

  4. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    6 publications · 721 citations

    6

    h-index

  5. MV
    Marta Volonteri

    Institut d'Astrophysique de Paris, France

    5 publications · 746 citations

    5

    h-index

1–5 of 530

Venues

  1. Monthly Notices of the Royal Astronomical Society

    60 publications · 6.8K citations

    36

    h-index

  2. The Astrophysical Journal

    ApJ · 36 publications · 8.8K citations

    31

    h-index

  3. Astronomy and Astrophysics

    19 publications · 1.1K citations

    17

    h-index

  4. Nature

    4 publications · 1.3K citations

    4

    h-index

  5. Meteoritics and Planetary Science

    3 publications · 325 citations

    3

    h-index

1–5