Magnetically Controlled Stellar Winds

Magnetically Controlled Stellar Winds is a theoretical construct in astrophysics that models stellar winds as outflows of ionized particles whose dynamics, geometry, and mass-loss rates are dominantly regulated by the large-scale magnetic field of the host star.

50

Publications

3K

Citations

101

Authors

72

Institutions

Publications per year

2017–2026

11

Authors

101

  1. SN
    S. N. Shore

    University of Pisa, Italy

    3 publications · 128 citations

    3

    h-index

  2. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 163 citations

    3

    h-index

  3. SP
    S. P. Owocki

    University of Delaware, United States

    3 publications · 406 citations

    3

    h-index

  4. CA
    Christopher A. Tout

    Institute of Astronomy, Russia

    2 publications · 91 citations

    2

    h-index

  5. RH
    R. H. D. Townsend

    University of Wisconsin–Madison, United States

    2 publications · 265 citations

    2

    h-index

1–5 of 101

Venues

  1. The Astrophysical Journal

    ApJ · 17 publications · 1.2K citations

    15

    h-index

  2. 10

    h-index

  3. The Astronomical Journal

    AJ · 3 publications · 128 citations

    3

    h-index

  4. Reports on Progress in Physics

    2 publications · 77 citations

    2

    h-index

  5. Space Science Reviews

    2 publications · 143 citations

    2

    h-index

1–5