Pre-main-sequence Disk Evolution

Pre-Main-Sequence Disk Evolution is a theoretical framework that describes the dynamic processes of mass accretion, angular momentum transport, and dust coagulation in protoplanetary disks surrounding young stellar objects during the pre-main-sequence phase of stellar evolution.

126

Publications

14.6K

Citations

490

Authors

289

Institutions

Publications per year

2017–2026

18

Authors

490

  1. NC
    Nuria Calvet

    University of Michigan, United States

    8 publications · 2.3K citations

    8

    h-index

  2. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    7 publications · 2.2K citations

    7

    h-index

  3. AN
    A. Natta

    Arcetri Astrophysical Observatory, Italy

    6 publications · 1.1K citations

    6

    h-index

  4. CF
    C. F. Manara

    European Southern Observatory, Germany

    6 publications · 743 citations

    6

    h-index

  5. PD
    Paola D’Alessio

    Universidad Nacional Autónoma de México, Mexico

    6 publications · 2.2K citations

    6

    h-index

1–5 of 490

Venues

  1. The Astrophysical Journal

    ApJ · 54 publications · 7.7K citations

    40

    h-index

  2. Astronomy and Astrophysics

    23 publications · 1.4K citations

    19

    h-index

  3. 7

    h-index

  4. The Astrophysical Journal Letters

    5 publications · 343 citations

    5

    h-index

  5. Annual Review of Astronomy and Astrophysics

    3 publications · 973 citations

    3

    h-index

1–5