Magnetically Driven Stellar Winds

Magnetically Driven Stellar Winds is a theoretical model of stellar mass loss in which the acceleration and structuring of outflowing plasma are predominantly governed by magnetic fields originating from the stellar interior, distinguishing it from thermally or radiatively driven wind mechanisms.

248

Publications

19.5K

Citations

505

Authors

337

Institutions

Publications per year

2017–2026

54

Authors

505

  1. AA
    A. A. Vidotto

    Trinity College Dublin, Ireland

    9 publications · 596 citations

    9

    h-index

  2. AU
    Asif ud‐Doula

    Pennsylvania State University, United States

    9 publications · 896 citations

    9

    h-index

  3. SP
    S. P. Owocki

    University of Delaware, United States

    8 publications · 928 citations

    8

    h-index

  4. TA
    Todd A. Thompson

    The Ohio State University, United States

    7 publications · 897 citations

    7

    h-index

  5. RH
    R. H. D. Townsend

    University of Wisconsin–Madison, United States

    6 publications · 752 citations

    6

    h-index

1–5 of 505

Venues

  1. The Astrophysical Journal

    ApJ · 103 publications · 9.4K citations

    49

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    65 publications · 4.1K citations

    36

    h-index

  3. Astronomy and Astrophysics

    16 publications · 672 citations

    15

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 609 citations

    8

    h-index

  5. The Astronomical Journal

    AJ · 6 publications · 249 citations

    6

    h-index

1–5