Red Supergiants
Red Supergiants is a stellar evolutionary phase representing massive stars that have exhausted core hydrogen and expanded into luminous, cool supergiants characterized by low surface temperatures and high luminosities following hydrogen shell burning and core contraction.
840
Publications
54.1K
Citations
2K
Authors
641
Institutions
Publications per year
2017–2026
213
Variants
Red Supergiant Stars
Parents
840
Grids of stellar models with rotation
Sylvia Ekström, C. Georgy, P. Eggenberger et al. · Astronomy and Astrophysics · 2011 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
3C 273 : A Star-Like Object with Large Red-Shift
Maarten Schmidt · Nature · 1963 · 1K citations · Full text
Natural Sciences, Astronomy, Physics +12
NUCLEOSYNTHESIS AND EVOLUTION OF MASSIVE METAL-FREE STARS
Alexander Heger, S. E. Woosley · The Astrophysical Journal · 2010 · 700 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 840
2K
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641

Centre National de la Recherche Scientifique
Paris, France
46 h-index
221 publications
19.6K citations
California Institute of Technology
Pasadena, United States
43 h-index
190 publications
11.6K citations

Space Telescope Science Institute
Baltimore, United States
34 h-index
100 publications
7.9K citations
University of Cambridge
Cambridge, United Kingdom
33 h-index
80 publications
7.8K citations
University of California, Berkeley
Berkeley, United States
33 h-index
95 publications
7.8K citations

University of Hawaii System
Honolulu, United States
31 h-index
87 publications
6.3K citations
KU Leuven
Leuven, Belgium
29 h-index
138 publications
9.6K citations

Kitt Peak National Observatory
Tucson, United States
27 h-index
41 publications
3.9K citations
1–8 of 641
ApJ · 253 publications · 16.5K citations
73
h-index
130 publications · 10.8K citations
56
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126 publications · 8.4K citations
47
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AJ · 89 publications · 4.1K citations
38
h-index
30 publications · 1.9K citations
25
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1–5