Eclipsing Binary Systems
Eclipsing Binary Systems is a subclass of binary star systems in which the orbital plane is oriented such that, from the perspective of the observer, one star periodically passes in front of the other, causing measurable dips in the system’s light curve due to mutual eclipses.
983
Publications
45.5K
Citations
2.5K
Authors
723
Institutions
Publications per year
2017–2026
155
983
An eclipsing-binary distance to the Large Magellanic Cloud accurate to two per cent
G. Pietrzyński, D. Graczyk, W. Gieren et al. · Nature · 2013 · 685 citations · Full text
1–5 of 983
2.5K
19
h-index
Center for Astrophysics Harvard & Smithsonian, United States
23 publications · 1.8K citations
19
h-index
18
h-index
17
h-index
Center for Astrophysics Harvard & Smithsonian, United States
16 publications · 1.3K citations
16
h-index
1–5 of 2.5K
723
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
34 h-index
156 publications
11K citations

University of Warwick
Coventry, United Kingdom
27 h-index
131 publications
5.5K citations

Villanova University
Radnor, United States
26 h-index
91 publications
12.7K citations
California Institute of Technology
Pasadena, United States
26 h-index
97 publications
6.5K citations

Keele University
Newcastle-under-Lyme, United Kingdom
26 h-index
78 publications
5K citations
Konkoly Observatory
Budapest, Hungary
24 h-index
50 publications
2.2K citations
University of Liège
Liège, Belgium
22 h-index
61 publications
3.1K citations

Chinese Academy of Sciences
Beijing, China
22 h-index
165 publications
4.1K citations
1–8 of 723
ApJ · 166 publications · 12.8K citations
52
h-index
174 publications · 6.7K citations
43
h-index
AJ · 134 publications · 7.3K citations
38
h-index
138 publications · 4.7K citations
36
h-index
57 publications · 1.8K citations
22
h-index
1–5