Accretion Of Solids

Accretion of Solids is a theoretical construct in planetary formation that describes the process by which microscopic dust particles in a protoplanetary disk coalesce under mutual gravitational and collisional interactions to form progressively larger solid bodies, ultimately leading to planetesimals.

264

Publications

27.3K

Citations

523

Authors

292

Institutions

Publications per year

2017–2026

88

Authors

523

  1. YA
    Y. Alibert

    University of Bern, Switzerland

    11 publications · 729 citations

    11

    h-index

  2. CW
    Chris W. Ormel

    University of Amsterdam, Netherlands

    8 publications · 562 citations

    8

    h-index

  3. AJ
    Anders Johansen

    Lund University, Sweden

    7 publications · 2K citations

    7

    h-index

  4. SJ
    S. J. Weidenschilling

    Planetary Science Institute, United States

    6 publications · 318 citations

    6

    h-index

  5. RM
    R. M. Canup

    Southwest Research Institute, United States

    6 publications · 938 citations

    6

    h-index

1–5 of 523

Venues

  1. The Astrophysical Journal

    ApJ · 38 publications · 3.4K citations

    31

    h-index

  2. Astronomy and Astrophysics

    36 publications · 3.7K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.1K citations

    18

    h-index

  4. Icarus

    22 publications · 4.6K citations

    17

    h-index

  5. Earth and Planetary Science Letters

    17 publications · 1.7K citations

    16

    h-index

1–5