Main-sequence Lifetime Effects

Main-Sequence Lifetime Effects is a theoretical construct in astrophysics that characterizes the influence of a star's duration in the hydrogen-burning phase on the long-term environmental stability and potential for life development on orbiting exoplanets.

27

Publications

1.8K

Citations

69

Authors

72

Institutions

Publications per year

2017–2026

3

Authors

69

  1. GM
    G. Michaud

    Université de Montréal, Canada

    4 publications · 287 citations

    4

    h-index

  2. JR
    J. Richer

    Université de Montréal, Canada

    3 publications · 264 citations

    3

    h-index

  3. JB
    J. Ballot

    Centre National de la Recherche Scientifique, France

    3 publications · 285 citations

    3

    h-index

  4. VS
    V. Silva Aguirre

    Aarhus University, Denmark

    3 publications · 285 citations

    3

    h-index

  5. AS
    Aldo Serenelli

    Aarhus University, Denmark

    3 publications · 285 citations

    3

    h-index

1–5 of 69

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 653 citations

    11

    h-index

  2. Astronomy and Astrophysics

    4 publications · 209 citations

    4

    h-index

  3. 4

    h-index

  4. arXiv (Cornell University)

    Repository · 2 publications · 99 citations

    2

    h-index

  5. DIGITAL.CSIC (Spanish National Research Council (CSIC))

    Repository · 1 publications · 136 citations

    1

    h-index

1–5