Convective Envelope

Convective Envelope is a stellar structural layer in which energy is transported primarily by convection, distinguishing it from radiative zones where energy moves through radiation rather than bulk fluid motion.

414

Publications

28.3K

Citations

823

Authors

395

Institutions

Publications per year

2017–2026

84

Parents

Authors

823

  1. LS
    L. Siess

    Université Libre de Bruxelles, Belgium

    10 publications · 1K citations

    10

    h-index

  2. JC
    J. Christensen‐Dalsgaard

    Aarhus University, Denmark

    9 publications · 1.7K citations

    9

    h-index

  3. CA
    Christopher A. Tout

    Institute of Astronomy, Russia

    9 publications · 439 citations

    9

    h-index

  4. JC
    John C. Lattanzio

    Monash University, Australia

    8 publications · 894 citations

    8

    h-index

  5. MB
    M. Busso

    University of Perugia, Italy

    8 publications · 747 citations

    8

    h-index

1–5 of 823

Venues

  1. The Astrophysical Journal

    ApJ · 145 publications · 12.9K citations

    65

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    75 publications · 4.4K citations

    34

    h-index

  3. Astronomy and Astrophysics

    58 publications · 2.6K citations

    30

    h-index

  4. arXiv (Cornell University)

    Repository · 10 publications · 253 citations

    10

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 268 citations

    9

    h-index

1–5