Stellar Accretion

Stellar Accretion is a physical process in astrophysics wherein matter, primarily gas and dust from an orbiting accretion disk, gravitationally collapses onto a forming or evolving star, distinguishing it from other accretion phenomena by its central role in stellar mass growth and energy release during star formation.

600

Publications

67.7K

Citations

1.2K

Authors

432

Institutions

Publications per year

2017–2026

60

Authors

1.2K

  1. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    23 publications · 4.5K citations

    23

    h-index

  2. NC
    Nuria Calvet

    University of Michigan, United States

    15 publications · 2.7K citations

    15

    h-index

  3. SJ
    Scott J. Kenyon

    Smithsonian Astrophysical Observatory, United States

    13 publications · 1.9K citations

    13

    h-index

  4. ML
    Mario Livio

    Space Telescope Science Institute, United States

    10 publications · 815 citations

    10

    h-index

  5. FK
    Frederick K. Lamb

    University of Illinois Urbana-Champaign, United States

    9 publications · 2.6K citations

    9

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 388 publications · 42.7K citations

    92

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    61 publications · 8.8K citations

    37

    h-index

  3. Astronomy and Astrophysics

    35 publications · 3.3K citations

    25

    h-index

  4. The Astronomical Journal

    AJ · 15 publications · 601 citations

    15

    h-index

  5. The Astrophysical Journal Supplement Series

    13 publications · 4.4K citations

    12

    h-index

1–5