Mass-loss Processes

Mass-Loss Processes is a theoretical construct in stellar astrophysics that refers to the mechanisms by which pre-main sequence stars eject material from their outer layers through winds, jets, and disk outflows, thereby reducing their mass during early evolutionary stages.

1.3K

Publications

88.8K

Citations

3.3K

Authors

920

Institutions

Publications per year

2017–2026

264

Authors

3.3K

  1. JS
    J. S. Vink

    Armagh Observatory & Planetarium, United Kingdom

    27 publications · 3.2K citations

    23

    h-index

  2. AD
    A. de Koter

    University of Amsterdam, Netherlands

    26 publications · 3K citations

    22

    h-index

  3. HO
    H. Olofsson

    Chalmers University of Technology, Sweden

    23 publications · 1.7K citations

    19

    h-index

  4. LD
    L. Decin

    KU Leuven, Belgium

    23 publications · 1.2K citations

    18

    h-index

  5. AA
    A. A. Zijlstra

    University of Manchester, United Kingdom

    18 publications · 741 citations

    16

    h-index

1–5 of 3.3K

Venues

  1. The Astrophysical Journal

    ApJ · 420 publications · 35.2K citations

    90

    h-index

  2. Astronomy and Astrophysics

    190 publications · 15K citations

    67

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    233 publications · 15.1K citations

    64

    h-index

  4. The Astronomical Journal

    AJ · 36 publications · 1.7K citations

    25

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 30 publications · 1.9K citations

    22

    h-index

1–5