Baryonic Processes

Baryonic Processes is a theoretical construct in astrophysics that encompasses the physical mechanisms governing the behavior and evolution of ordinary matter—such as gas cooling, star formation, supernova feedback, and chemical enrichment—within galaxies, distinguishing it from dark matter dynamics and large-scale gravitational processes in galaxy formation models.

1K

Publications

91.4K

Citations

9.6K

Authors

930

Institutions

Publications per year

2017–2026

283

Authors

9.6K

  1. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    19 publications · 6.2K citations

    19

    h-index

  2. MV
    Mark Vogelsberger

    Center for Astrophysics Harvard & Smithsonian, United States

    18 publications · 6.1K citations

    17

    h-index

  3. VS
    Volker Springel

    Max Planck Institute for Astrophysics, Germany

    15 publications · 6.9K citations

    15

    h-index

  4. IG
    Ian G. McCarthy

    Liverpool John Moores University, United Kingdom

    15 publications · 1.2K citations

    15

    h-index

  5. JS
    Joop Schaye

    Leiden University, Netherlands

    15 publications · 1.9K citations

    15

    h-index

1–5 of 9.6K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    211 publications · 22.9K citations

    77

    h-index

  2. The Astrophysical Journal

    ApJ · 104 publications · 15.7K citations

    56

    h-index

  3. Physics Letters B

    97 publications · 5.3K citations

    39

    h-index

  4. Physical Review Letters

    PRL · 34 publications · 5.2K citations

    27

    h-index

  5. 27

    h-index

1–5