Wide Binary Formation
Wide Binary Formation is a theoretical framework in astrophysics that explains the gravitational pairing and subsequent evolution of binary star systems with separations exceeding 1000 astronomical units, distinguishing it from closer binary formation mechanisms by emphasizing dynamical capture and environmental perturbations in sparse stellar nurseries.
58
Publications
4.4K
Citations
228
Authors
144
Institutions
Publications per year
2017–2026
18
Parents
58
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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144
Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
5 publications
209 citations

Institute for Advanced Study
Princeton, United States
5 h-index
10 publications
364 citations
California Institute of Technology
Pasadena, United States
5 h-index
7 publications
860 citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
4 h-index
5 publications
566 citations
The University of Tokyo
Tokyo, Japan
4 h-index
15 publications
1.7K citations

Johns Hopkins University
Baltimore, United States
3 h-index
7 publications
344 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
3 h-index
12 publications
459 citations
Technion – Israel Institute of Technology
Haifa, Israel
3 h-index
7 publications
169 citations
1–8 of 144
ApJ · 17 publications · 1.8K citations
16
h-index
14 publications · 717 citations
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AJ · 6 publications · 241 citations
6
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5 publications · 270 citations
5
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3 publications · 64 citations
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