Wide Binary Stars
Wide Binary Stars is a binary star system characterized by a large physical separation between the two constituent stars, typically exceeding 1,000 astronomical units, resulting in weak gravitational interaction and nearly independent evolutionary trajectories.
127
Publications
7.8K
Citations
363
Authors
204
Institutions
Publications per year
2017–2026
43
Parents
127
A Wide Symbiotic Channel to Type Ia Supernovae
The Astrophysical Journal · 1999 · 388 citations · Full text
Natural Sciences, Astronomy, Physics +17
The Formation and Fragmentation of Disks Around Primordial Protostars
Paul C. Clark, Simon C. O. Glover, Rowan J. Smith et al. · Science · 2011 · 387 citations · Full text
Natural Sciences, Astronomy, Physics +17
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204
Max Planck Institute for Astronomy
Heidelberg, Germany
13 h-index
20 publications
1.1K citations
California Institute of Technology
Pasadena, United States
6 h-index
10 publications
1.1K citations
University of California, Berkeley
Berkeley, United States
6 h-index
6 publications
361 citations
The University of Texas at Austin
Austin, United States
6 h-index
13 publications
1.1K citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
12 publications
636 citations
Princeton University
Princeton, United States
5 h-index
7 publications
571 citations

Institute for Advanced Study
Princeton, United States
5 h-index
7 publications
378 citations
Queen Mary University of London
London, United Kingdom
4 h-index
9 publications
320 citations
1–8 of 204
ApJ · 36 publications · 3K citations
27
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30 publications · 1.6K citations
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AJ · 10 publications · 524 citations
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8 publications · 297 citations
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Repository · 4 publications · 102 citations
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