Main-sequence Structure
Main-Sequence Structure is a theoretical astrophysical model that characterizes the internal physical and compositional organization of stars in hydrostatic equilibrium during the phase of core hydrogen fusion, distinguished from other stellar models by its reliance on mass-dependent relationships between temperature, pressure, luminosity, and energy transport mechanisms governing stellar stability and evolution.
210
Publications
14.6K
Citations
616
Authors
282
Institutions
Publications per year
2017–2026
34
Parents
210
Model and theoretical seismicity
Robert Burridge, L. Knopoff · Bulletin of the Seismological Society of America · 1967 · 1.5K citations
Centauri: The Population Puzzle Goes Deeper
L. R. Bedin, G. Piotto, Jay Anderson et al. · The Astrophysical Journal · 2004 · 564 citations · Full text
Natural Sciences, Astronomy, Physics +17
OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event
I. A. Bond, A. Udalski, M. Jaroszyski et al. · The Astrophysical Journal · 2004 · 392 citations · Full text
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282

Space Telescope Science Institute
Baltimore, United States
16 h-index
33 publications
3.5K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
42 publications
3.8K citations
Osservatorio Astronomico di Padova
Padua, Italy
12 h-index
20 publications
1.9K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
12 h-index
18 publications
1.8K citations

University of Padua
Padua, Italy
11 h-index
17 publications
4.7K citations
Yale University
New Haven, United States
11 h-index
20 publications
1.5K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
9 h-index
14 publications
1.2K citations
Harvard University
Cambridge, United States
8 h-index
11 publications
799 citations
1–8 of 282
ApJ · 61 publications · 5.1K citations
32
h-index
30 publications · 2.1K citations
21
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AJ · 27 publications · 1.5K citations
19
h-index
20 publications · 1.3K citations
18
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PASP · 9 publications · 236 citations
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