Close Binary Formation
Close Binary Formation is a theoretical framework within the study of binary star formation that specifically accounts for the dynamical processes and physical conditions leading to the emergence of binary systems with orbital separations typically less than a few astronomical units.
309
Publications
20.3K
Citations
754
Authors
376
Institutions
Publications per year
2017–2026
56
Parents
309
A Wide Symbiotic Channel to Type Ia Supernovae
The Astrophysical Journal · 1999 · 388 citations · Full text
Natural Sciences, Astronomy, Physics +17
Kepler-47: A Transiting Circumbinary Multiplanet System
Jerome A. Orosz, William F. Welsh, Joshua A. Carter et al. · Science · 2012 · 379 citations · Full text
Natural Sciences, Astronomy, Physics +16
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376
Institute of Astronomy
Moscow, Russia
15 h-index
32 publications
3.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
13 h-index
23 publications
4.9K citations
California Institute of Technology
Pasadena, United States
11 h-index
27 publications
1.6K citations
Friedrich-Alexander-Universität Erlangen-Nürnberg
Erlangen, Germany
10 h-index
29 publications
2.1K citations
University of Arizona
Tucson, United States
10 h-index
13 publications
1.4K citations

Chinese Academy of Sciences
Beijing, China
9 h-index
25 publications
819 citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
24 publications
814 citations
University of Hertfordshire
Hatfield, United Kingdom
8 h-index
10 publications
390 citations
1–8 of 376
ApJ · 74 publications · 7.1K citations
48
h-index
57 publications · 3.5K citations
31
h-index
36 publications · 2.6K citations
25
h-index
11 publications · 479 citations
11
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10 publications · 516 citations
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