White Dwarfs
White Dwarf is a stellar remnant constituting the final evolutionary state of low- to intermediate-mass stars, distinguished by its high density, electron-degenerate core, and lack of active nuclear fusion.
7.9K
Publications
507K
Citations
11.7K
Authors
1.9K
Institutions
Publications per year
2017–2026
1.7K
7.9K
The Luminosity Function and Stellar Evolution.
E. E. Salpeter · The Astrophysical Journal · 1955 · 8.7K citations
Natural Sciences, Astronomy, Physics +16
A Massive Pulsar in a Compact Relativistic Binary
John Antoniadis, P. C. C. Freire, Norbert Wex et al. · Science · 2013 · 3.8K citations · Full text
Natural Sciences, Astronomy, Physics +17
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Jieun Choi, Aaron Dotter, Charlie Conroy et al. · The Astrophysical Journal · 2016 · 2.8K citations · Full text
Natural Sciences, Astronomy, Physics +14
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1.9K

University of Warwick
Coventry, United Kingdom
88 h-index
1.3K publications
80.4K citations
Max Planck Institute for Astrophysics
Garching, Germany
83 h-index
535 publications
60.7K citations
University of California, Berkeley
Berkeley, United States
81 h-index
509 publications
57.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
81 h-index
634 publications
68K citations
The University of Texas at Austin
Austin, United States
79 h-index
736 publications
47K citations
California Institute of Technology
Pasadena, United States
76 h-index
867 publications
60K citations

Centre National de la Recherche Scientifique
Paris, France
75 h-index
834 publications
58.9K citations

Space Telescope Science Institute
Baltimore, United States
74 h-index
587 publications
34.9K citations
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ApJ · 2.6K publications · 192.7K citations
177
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1.7K publications · 86.5K citations
122
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746 publications · 38.9K citations
94
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AJ · 349 publications · 17.6K citations
67
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125 publications · 31.3K citations
65
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