Protoplanetary Disk Evolution

Protoplanetary Disk Evolution is the process by which a rotating circumstellar disk of gas and dust undergoes structural, thermal, and compositional changes over time due to gravitational, radiative, and hydrodynamic interactions, ultimately governing the conditions for planetary formation and early system architecture.

1.1K

Publications

89.1K

Citations

2.1K

Authors

690

Institutions

Publications per year

2017–2026

463

Authors

2.1K

  1. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    25 publications · 2.8K citations

    24

    h-index

  2. GR
    Giovanni Rosotti

    Leiden University, Netherlands

    25 publications · 1.4K citations

    21

    h-index

  3. MB
    Martin Bizzarro

    University of Copenhagen, Denmark

    23 publications · 3.4K citations

    21

    h-index

  4. TB
    T. Birnstiel

    Ludwig-Maximilians-Universität München, Germany

    22 publications · 3.4K citations

    20

    h-index

  5. AN
    Alexander N. Krot

    University of Hawaiʻi at Mānoa, United States

    20 publications · 2.9K citations

    19

    h-index

1–5 of 2.1K

Venues

  1. The Astrophysical Journal

    ApJ · 271 publications · 23.4K citations

    88

    h-index

  2. Astronomy and Astrophysics

    199 publications · 14.2K citations

    68

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    116 publications · 7.4K citations

    50

    h-index

  4. The Astrophysical Journal Letters

    46 publications · 3.9K citations

    34

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 39 publications · 1.8K citations

    25

    h-index

1–5