Overcontact Binary Stars
Overcontact Binary Stars is a type of close binary star system in which both component stars fill and share a common outer envelope, resulting in continuous mass transfer and synchronized orbital and rotational motion due to their deeply interacting configurations.
43
Publications
2.8K
Citations
136
Authors
92
Institutions
Publications per year
2017–2026
4
Variants
W Uma StarsW Ursae Majoris Variables
Parents
43
A new route towards merging massive black holes
Pablo Marchant, N. Langer, Philipp Podsiadlowski et al. · Astronomy and Astrophysics · 2016 · 620 citations · Full text
Natural Sciences, Astronomy, Physics +17
Deep, Low Mass Ratio Overcontact Binary Systems. III. CU Tauri and TV Muscae
S. Qian, Yunfei Yang, Boonrucksar Soonthornthum et al. · The Astronomical Journal · 2005 · 102 citations · Full text
Natural Sciences, Astronomy, Physics +13
1–5 of 43
136
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10
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10
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6
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1–5 of 136
92
National Astronomical Observatories
Beijing, China
20 h-index
74 publications
3.8K citations

Chinese Academy of Sciences
Beijing, China
20 h-index
93 publications
4.3K citations

Yunnan Observatories
Kunming, China
8 h-index
37 publications
1.1K citations
University of Chinese Academy of Sciences
Beijing, China
5 h-index
17 publications
339 citations

Chiang Mai University
Chiang Mai, Thailand
5 h-index
5 publications
321 citations
National Astronomical Research Institute of Thailand
Chiang Mai, Thailand
5 h-index
6 publications
221 citations
Huaibei Normal University
Huaibei, China
4 h-index
5 publications
284 citations

Ankara University
Ankara, Türkiye
3 h-index
11 publications
290 citations
1–8 of 92
AJ · 22 publications · 1.5K citations
19
h-index
ApJ · 5 publications · 163 citations
5
h-index
5 publications · 770 citations
5
h-index
4 publications · 190 citations
4
h-index
3 publications · 59 citations
3
h-index
1–5