Blue Supergiants
Blue Supergiants is a stellar classification denoting a massive, luminous star in the late evolutionary phase characterized by high surface temperatures and spectral types O or B, distinguished from other supergiants by its prominent blue color and position on the upper left portion of the Hertzsprung-Russell diagram.
328
Publications
18.2K
Citations
718
Authors
375
Institutions
Publications per year
2017–2026
66
Variants
Blue Supergiant
Parents
328
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
A temperate rocky super-Earth transiting a nearby cool star
Jason Dittmann, Jonathan Irwin, David Charbonneau et al. · Nature · 2017 · 353 citations · Full text
Natural Sciences, Astronomy, Physics +12
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375

University of Concepción
Concepción, Chile
17 h-index
35 publications
1.9K citations

University of Hawaii System
Honolulu, United States
16 h-index
41 publications
2K citations
University of California, Berkeley
Berkeley, United States
16 h-index
32 publications
3.5K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
19 publications
2.7K citations

University of Minnesota
Minneapolis, United States
11 h-index
15 publications
1.4K citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
10 h-index
22 publications
1K citations
University of Geneva
Geneva, Switzerland
10 h-index
22 publications
2.5K citations

Armagh Observatory & Planetarium
Armagh, United Kingdom
10 h-index
21 publications
1.2K citations
1–8 of 375
ApJ · 88 publications · 6.1K citations
40
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48 publications · 2.5K citations
28
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44 publications · 2.1K citations
28
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AJ · 40 publications · 1.7K citations
26
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Repository · 10 publications · 418 citations
10
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