Contact Binary Stars
Contact Binary Stars is a type of binary star system in which two stellar components orbit so closely that their outer atmospheres physically interact and share a common envelope, distinguishing it from detached or semi-detached systems by direct mass and energy exchange between the stars.
315
Publications
14.3K
Citations
926
Authors
385
Institutions
Publications per year
2017–2026
72
Variants
Contact Binaries
Parents
315
On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko
H. Sierks, C. Barbieri, P. Lamy et al. · Science · 2015 · 437 citations
Natural Sciences, Astronomy, Physics +15
The Structure of Contact Binaries
L. B. Lucy · The Astrophysical Journal · 1968 · 357 citations
Natural Sciences, Astronomy, Physics +13
Evolution of Close Binary Systems
K. Yakut, P. P. Eggleton · The Astrophysical Journal · 2005 · 350 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 315
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385

Chinese Academy of Sciences
Beijing, China
24 h-index
241 publications
6.7K citations

University of Toronto
Toronto, Canada
22 h-index
40 publications
2.6K citations

Yunnan Observatories
Kunming, China
20 h-index
171 publications
5.2K citations
University of Chinese Academy of Sciences
Beijing, China
18 h-index
104 publications
3.2K citations
National Astronomical Observatories
Beijing, China
18 h-index
100 publications
2.5K citations

Andrews University
Berrien Springs, United States
13 h-index
22 publications
866 citations
National Astronomical Research Institute of Thailand
Chiang Mai, Thailand
12 h-index
33 publications
732 citations
Shandong University
Jinan, China
10 h-index
44 publications
2.1K citations
1–8 of 385
ApJ · 44 publications · 3.2K citations
31
h-index
64 publications · 2.9K citations
28
h-index
AJ · 56 publications · 2.3K citations
28
h-index
17 publications · 576 citations
15
h-index
13 publications · 248 citations
12
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1–5