Radiation-driven Stellar Winds

Radiation-Driven Stellar Winds is a theoretical model in astrophysics describing a type of stellar mass loss mechanism in which radiation pressure exerted by photons in the outer layers of massive stars accelerates material to supersonic velocities through momentum transfer, distinguishing it from other stellar wind mechanisms by its primary reliance on radiative forces rather than thermal or magnetic processes.

428

Publications

29.9K

Citations

794

Authors

341

Institutions

Publications per year

2017–2026

85

Authors

794

  1. SP
    S. P. Owocki

    University of Delaware, United States

    27 publications · 2.4K citations

    20

    h-index

  2. JP
    J. Puls

    Ludwig-Maximilians-Universität München, Germany

    14 publications · 797 citations

    13

    h-index

  3. AW
    A. W. A. Pauldrach

    Ludwig-Maximilians-Universität München, Germany

    15 publications · 1.2K citations

    13

    h-index

  4. JO
    J. O. Sundqvist

    KU Leuven, Belgium

    10 publications · 440 citations

    11

    h-index

  5. JS
    J. S. Vink

    Armagh Observatory & Planetarium, United Kingdom

    10 publications · 862 citations

    10

    h-index

1–5 of 794

Venues

  1. The Astrophysical Journal

    ApJ · 173 publications · 14.8K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    70 publications · 5.3K citations

    38

    h-index

  3. Astronomy and Astrophysics

    67 publications · 4.5K citations

    37

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 298 citations

    9

    h-index

  5. ArXiv.org

    Repository · 9 publications · 344 citations

    9

    h-index

1–5