Rotational Mixing

Rotational Mixing is a stellar astrophysical process in which angular momentum and chemical elements are redistributed within a star due to rotation-induced hydrodynamic instabilities and shear flows, thereby modifying its internal composition and evolution.

290

Publications

21.3K

Citations

595

Authors

330

Institutions

Publications per year

2017–2026

43

Authors

595

  1. NL
    N. Langer

    University of Bonn, Germany

    21 publications · 3.4K citations

    18

    h-index

  2. GM
    G. Meynet

    University of Geneva, Switzerland

    17 publications · 1.9K citations

    16

    h-index

  3. AM
    A. Maeder

    Global Social Observatory, Switzerland

    15 publications · 1.3K citations

    14

    h-index

  4. CC
    C. Charbonnel

    Centre National de la Recherche Scientifique, France

    13 publications · 1.5K citations

    13

    h-index

  5. IB
    I. Brott

    University of Vienna, Austria

    11 publications · 2.3K citations

    11

    h-index

1–5 of 595

Venues

  1. Astronomy and Astrophysics

    65 publications · 7.1K citations

    41

    h-index

  2. The Astrophysical Journal

    ApJ · 49 publications · 4.5K citations

    31

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    27 publications · 2.1K citations

    22

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 14 publications · 1.1K citations

    13

    h-index

  5. arXiv (Cornell University)

    Repository · 6 publications · 159 citations

    6

    h-index

1–5