Galactic Circulation

Galactic Circulation is a theoretical framework within astrophysics that characterizes the large-scale movement and recycling of baryonic matter between the interstellar medium and the galactic halo, distinguished by its focus on feedback-driven outflows and coherent inflows regulating star formation and chemical evolution in galaxies.

10

Publications

323

Citations

17

Authors

11

Institutions

Publications per year

2017–2026

1

Authors

17

  1. BR
    B. R. Dawson

    The University of Adelaide, Australia

    1 publications · 10 citations

    1

    h-index

  2. AD
    Avishai Dekel

    Hebrew University of Jerusalem, Israel

    1 publications · 78 citations

    1

    h-index

  3. MM
    M.A. McDonough

    University of Oxford, United Kingdom

    1 publications · 10 citations

    1

    h-index

  4. VA
    V. Antonuccio-Delogu

    Osservatorio Astrofisico di Catania, Italy

    1 publications · 40 citations

    1

    h-index

  5. ER
    E. R. Harrison

    University of Massachusetts Amherst, United States

    1 publications · 22 citations

    1

    h-index

1–5 of 17

Venues

  1. 3

    h-index

  2. Nature

    2 publications · 89 citations

    2

    h-index

  3. Reports in Advances of Physical Sciences

    1 publications · 12 citations

    1

    h-index

  4. Scientific American

    1 publications · 13 citations

    1

    h-index

  5. Publications of the Astronomical Society of Australia

    PASA · 1 publications · 10 citations

    1

    h-index

1–5