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.
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2.7K
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283
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177
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2017–2026
8
Variants
Instability Strip
Parents
65
Classical Cepheid Pulsation Models. X. The Period‐Age Relation
G. Bono, M. Marconi, S. Cassisi et al. · The Astrophysical Journal · 2005 · 176 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Observatoire de Paris
Paris, France
8 h-index
16 publications
565 citations
University of Vienna
Vienna, Austria
7 h-index
18 publications
501 citations

Astronomical Observatory of Capodimonte
Naples, Italy
7 h-index
16 publications
945 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
22 publications
1.2K citations

Royal Observatory of Belgium
Brussels, Belgium
6 h-index
12 publications
254 citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
5 h-index
8 publications
311 citations
Instituto de Astrofísica de Andalucía
Granada, Spain
5 h-index
20 publications
432 citations

The University of Sydney
Sydney, Australia
5 h-index
10 publications
645 citations
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ApJ · 16 publications · 940 citations
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14 publications · 543 citations
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14 publications · 596 citations
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AJ · 3 publications · 93 citations
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2 publications · 57 citations
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