Wolf-rayet Progenitors

Wolf-Rayet Progenitors is a theoretical construct denoting a massive stellar progenitor system in a late evolutionary stage characterized by strong stellar winds and depleted hydrogen envelopes, specifically distinguished by its origin from a Wolf-Rayet star immediately prior to core-collapse supernova.

623

Publications

45.1K

Citations

1.3K

Authors

489

Institutions

Publications per year

2017–2026

90

Authors

1.3K

  1. PM
    Philip Massey

    Lowell Observatory, United States

    33 publications · 2.5K citations

    27

    h-index

  2. AF
    A. F. J. Moffat

    Université de Montréal, Canada

    43 publications · 1.8K citations

    25

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    31 publications · 3.1K citations

    25

    h-index

  4. PA
    P. A. Crowther

    University of Sheffield, United Kingdom

    25 publications · 1.5K citations

    22

    h-index

  5. WH
    W.‐R. Hamann

    University of Potsdam, Germany

    19 publications · 1.5K citations

    16

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 197 publications · 16.7K citations

    64

    h-index

  2. Astronomy and Astrophysics

    96 publications · 6.2K citations

    45

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    95 publications · 6.1K citations

    44

    h-index

  4. The Astronomical Journal

    AJ · 45 publications · 2.1K citations

    26

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 21 publications · 650 citations

    14

    h-index

1–5