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Activity of Contact Binary Systems
1985This review will consider various indicators of activity in contact binaries. We shall limit ourselves to late-type contact systems which are traditionally called the “W UMa-type” systems. This limitation results mainly from a better knowledge of properties of cooler systems (i.e.
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An investigation of contact and non-contact binary systems
1986Spectroscopic and photometric observations of six late-type contact and near-contact binaries are presented, and the results of the analyses discussed. Absolute dimensions have been deduced for three systems: YY Ceti. CX Aquarii and RV Corvi. YY Ceti, which has an orbital period of 0.79 days, is found to be composed of a normal main-sequence star of ...
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Spacecraft trajectory tracking and parameter estimation around a splitting contact binary asteroid
Acta Astronautica, 2020Tiago Silva +2 more
exaly
Contact angles of binary liquids and their interpretation
Journal of Adhesion Science and Technology, 1992A W Neumann
exaly
Orbital Motion in the Vicinity of the Non-collinear Equilibrium Points of a Contact Binary Asteroid
Planetary and Space Science, 2015Jinglang Feng
exaly
Changes in the orbital period of the near-contact binary BF Vir
Chinese Astronomy and Astrophysics, 2000Sheng-Bang Qian
exaly

