Stellar Evolution

Stellar Evolution is the astrophysical process that describes the systematic changes in a star’s internal structure, composition, and observable properties over its life cycle, from formation in a collapsing interstellar cloud through successive nuclear-burning phases to its final remnant state.

41.3K

Publications

3M

Citations

41.3K

Authors

3.9K

Institutions

Publications per year

2017–2026

8.7K

Authors

41.3K

  1. NL
    N. Langer

    University of Bonn, Germany

    225 publications · 27.8K citations

    83

    h-index

  2. GM
    G. Meynet

    University of Geneva, Switzerland

    182 publications · 20.6K citations

    75

    h-index

  3. RS
    Ralf S. Klessen

    Heidelberg University, Germany

    154 publications · 14.4K citations

    67

    h-index

  4. KN
    K. Nomoto

    The University of Tokyo, Japan

    122 publications · 18.8K citations

    64

    h-index

  5. AR
    A. Renzini

    Osservatorio Astronomico di Padova, Italy

    104 publications · 16.8K citations

    64

    h-index

1–5 of 41.3K

Venues

  1. The Astrophysical Journal

    ApJ · 10.9K publications · 916.3K citations

    342

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    7.3K publications · 514.5K citations

    250

    h-index

  3. Astronomy and Astrophysics

    5.7K publications · 379.4K citations

    226

    h-index

  4. Nature

    802 publications · 111.6K citations

    186

    h-index

  5. The Astronomical Journal

    AJ · 1.9K publications · 133.9K citations

    152

    h-index

1–5