Jet Collimation

Jet Collimation is a physical process in the context of Young Stellar Objects whereby bipolar outflows are constrained into narrow, highly directed streams by magnetic fields and disk-wind mechanisms, distinguishing it from uncollimated or isotropic mass ejections.

403

Publications

25.7K

Citations

1.1K

Authors

494

Institutions

Publications per year

2017–2026

66

Authors

1.1K

  1. AF
    Adam Frank

    University of Rochester, United States

    12 publications · 918 citations

    12

    h-index

  2. SC
    S. Cabrit

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    9 publications · 552 citations

    9

    h-index

  3. KT
    K. Tsinganos

    National and Kapodistrian University of Athens, Greece

    8 publications · 250 citations

    8

    h-index

  4. FB
    F. Bacciotti

    Arcetri Astrophysical Observatory, Italy

    8 publications · 531 citations

    8

    h-index

  5. EG
    Eric G. Blackman

    University of Rochester, United States

    7 publications · 584 citations

    7

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 132 publications · 9.3K citations

    56

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    56 publications · 3.6K citations

    34

    h-index

  3. Astronomy and Astrophysics

    45 publications · 2.4K citations

    29

    h-index

  4. The Astrophysical Journal Letters

    11 publications · 664 citations

    11

    h-index

  5. The Astronomical Journal

    AJ · 8 publications · 308 citations

    8

    h-index

1–5