Modelling of W UMa-type variable stars
W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand how these systems form and evolve requires observations spanning many years, followed by detailed models of as many of them as possible.
P. Skelton, D. Smits
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CCD photometric study of the short period contact binary CE Leonis [PDF]
Yulan Yang, Qingyao Liu
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Analysis and solution of the light and radial velocity curves of the contact binary TY Bootis
E. F. Milone+3 more
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TW Coronae Borealis: A Detached Near-Contact Binary System [PDF]
Xianshu Zhang, R.-X. Zhang
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On the performance of GAIA on photometry of eclipsing binaries: The case of four near-contact and contact systems [PDF]
P. G. Niarchos, V. N. Manimanis
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A contact binary satellite of the asteroid (152830) Dinkinesh. [PDF]
Levison HF+118 more
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PHOTOMETRIC SOLUTIONS AND SPOT MODEL OF THE CONTACT BINARY AB ANDROMEDAE [PDF]
Jae-Woo Kim Lee
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Impingement of suspending droplets with coming ones at different off-central distances: A molecular dynamics study. [PDF]
Sun L+5 more
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On a structure of a contact region in flows of a binary gas mixture
Noriko Umemura+3 more
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Photometric study of the contact binary star V861 Herculis [PDF]
Sz. Csizmadia+3 more
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