Wind Clumping

Wind Clumping is a phenomenon in astrophysical stellar winds wherein the outflowing material is distributed in dense, localized regions or parcels rather than being uniformly continuous, leading to deviations in observational diagnostics and mass-loss rate estimates.

84

Publications

5.3K

Citations

177

Authors

132

Institutions

Publications per year

2017–2026

15

Variants

Stellar Wind Clumping

Authors

177

  1. JO
    J. O. Sundqvist

    KU Leuven, Belgium

    8 publications · 474 citations

    8

    h-index

  2. JP
    J. Puls

    Ludwig-Maximilians-Universität München, Germany

    8 publications · 518 citations

    8

    h-index

  3. WH
    W.‐R. Hamann

    University of Potsdam, Germany

    5 publications · 324 citations

    5

    h-index

  4. JE
    J. E. Dyson

    University of Manchester, United Kingdom

    5 publications · 184 citations

    5

    h-index

  5. TW
    T. W. Hartquist

    University of Leeds, United Kingdom

    4 publications · 133 citations

    4

    h-index

1–5 of 177

Venues

  1. Astronomy and Astrophysics

    21 publications · 1.5K citations

    19

    h-index

  2. The Astrophysical Journal

    ApJ · 15 publications · 1.2K citations

    14

    h-index

  3. 14

    h-index

  4. arXiv (Cornell University)

    Repository · 3 publications · 210 citations

    3

    h-index

  5. The Astronomical Journal

    AJ · 3 publications · 129 citations

    3

    h-index

1–5