Subdwarf Stars
Subdwarf Stars is a stellar classification category denoting stars that lie below the main sequence in the Hertzsprung-Russell diagram and are distinguished by their lower luminosity and higher surface temperature compared to typical main-sequence stars of similar spectral type, often associated with evolved or metal-poor stellar populations.
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2017–2026
135
Variants
Subdwarf
609
Secondary standard stars for absolute spectrophotometry
J. B. Oke, James E. Gunn · The Astrophysical Journal · 1983 · 2.8K citations
Natural Sciences, Astronomy, Physics +13
The origin of subdwarf B stars - II
Zhanwen Han, Philipp Podsiadlowski, P. F. L. Maxted et al. · Monthly Notices of the Royal Astronomical Society · 2003 · 693 citations · Full text
Natural Sciences, Astronomy, Physics +17
U. Heber · Annual Review of Astronomy and Astrophysics · 2009 · 473 citations
Natural Sciences, Astronomy, Physics +17
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464
Friedrich-Alexander-Universität Erlangen-Nürnberg
Erlangen, Germany
34 h-index
207 publications
8.6K citations
University of Arizona
Tucson, United States
33 h-index
105 publications
7.3K citations
Université de Montréal
Montreal, Canada
30 h-index
121 publications
6.8K citations
KU Leuven
Leuven, Belgium
29 h-index
104 publications
4.7K citations

University of Warwick
Coventry, United Kingdom
29 h-index
70 publications
3.2K citations

Centre National de la Recherche Scientifique
Paris, France
27 h-index
66 publications
2.6K citations
Missouri State University
Springfield, United States
26 h-index
124 publications
3.9K citations

Armagh Observatory & Planetarium
Armagh, United Kingdom
24 h-index
69 publications
2.4K citations
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ApJ · 173 publications · 11.9K citations
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112 publications · 4.8K citations
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113 publications · 6.4K citations
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AJ · 48 publications · 3.3K citations
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15 publications · 686 citations
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