Classical Instability Strip

Classical Instability Strip is a theoretical region in the Hertzsprung-Russell diagram defined by specific temperature and luminosity ranges where post-main-sequence stars become dynamically unstable due to helium ionization-driven opacity mechanisms, enabling radial pulsations characteristic of classical Cepheid and RR Lyrae variable stars.

65

Publications

2.7K

Citations

283

Authors

177

Institutions

Publications per year

2017–2026

8

Variants

Instability Strip

Authors

283

  1. MM
    M. Marconi

    Astronomical Observatory of Capodimonte, Italy

    8 publications · 537 citations

    8

    h-index

  2. PL
    P. Lampens

    Royal Observatory of Belgium, Belgium

    5 publications · 94 citations

    5

    h-index

  3. AS
    Allan Sandage

    Carnegie Observatories, United States

    5 publications · 452 citations

    5

    h-index

  4. GT
    G. Tammann

    University of Basel, Switzerland

    5 publications · 452 citations

    5

    h-index

  5. AZ
    Ai-Ying Zhou

    National Astronomical Observatories, China

    4 publications · 57 citations

    4

    h-index

1–5 of 283

Venues

  1. The Astrophysical Journal

    ApJ · 16 publications · 940 citations

    15

    h-index

  2. Astronomy and Astrophysics

    14 publications · 543 citations

    13

    h-index

  3. 13

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 93 citations

    3

    h-index

  5. Astronomy and Astrophysics Supplement Series

    2 publications · 57 citations

    2

    h-index

1–5