Common-envelope Evolution

Common-Envelope Evolution is a critical phase in binary star dynamics wherein a binary star system undergoes rapid orbital shrinkage as a donor star—often a red giant or massive star—expands and transfers mass to its companion, leading to the formation of a shared gaseous envelope that envelopes both stars and drives spiral-in through drag forces, ultimately determining the fate of close compact binaries and supernova progenitors.

592

Publications

46.8K

Citations

1K

Authors

428

Institutions

Publications per year

2017–2026

216

Authors

1K

  1. NS
    Noam Soker

    Technion – Israel Institute of Technology, Israel

    38 publications · 3.5K citations

    28

    h-index

  2. PP
    Philipp Podsiadlowski

    University of Oxford, United Kingdom

    21 publications · 5.1K citations

    21

    h-index

  3. RE
    Ronald E. Taam

    Northwestern University, United States

    19 publications · 2.3K citations

    18

    h-index

  4. CA
    Christopher A. Tout

    Institute of Astronomy, Russia

    17 publications · 2.8K citations

    16

    h-index

  5. ZH
    Zhanwen Han

    Chinese Academy of Sciences, China

    17 publications · 3.2K citations

    16

    h-index

1–5 of 1K

Venues

  1. The Astrophysical Journal

    ApJ · 155 publications · 14.2K citations

    69

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    191 publications · 15.4K citations

    59

    h-index

  3. Astronomy and Astrophysics

    58 publications · 4.8K citations

    35

    h-index

  4. The Astrophysical Journal Letters

    20 publications · 1.4K citations

    20

    h-index

  5. arXiv (Cornell University)

    Repository · 16 publications · 737 citations

    14

    h-index

1–5