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
27
Eclipsing binaries in open clusters. II. V453Cyg in NGC6871 ⋆
J. Southworth, P. F. L. Maxted, B. Smalley · 2008 · 246 citations
Natural Sciences, Astronomy, Physics +13
Iron Convection Zones in B, A, and F Stars
O. Richard, G. Michaud, J. Richer · The Astrophysical Journal · 2001 · 142 citations · Full text
Natural Sciences, Astronomy, Physics +17
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72

Centre National de la Recherche Scientifique
Paris, France
6 h-index
11 publications
1.2K citations
Université de Montréal
Montreal, Canada
4 h-index
10 publications
815 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
5 publications
322 citations

Université Fédérale de Toulouse Midi-Pyrénées
Toulouse, France
3 h-index
4 publications
432 citations
Délégation Paris 7
Bagnolet, France
3 h-index
3 publications
269 citations
Consejo Superior de Investigaciones Científicas
Madrid, Spain
3 h-index
3 publications
285 citations
Max Planck Institute for Astrophysics
Garching, Germany
3 h-index
8 publications
708 citations
Université Paris Cité
Paris, France
3 h-index
3 publications
269 citations
1–8 of 72
ApJ · 11 publications · 653 citations
11
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4 publications · 209 citations
4
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4 publications · 217 citations
4
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Repository · 2 publications · 99 citations
2
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Repository · 1 publications · 136 citations
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