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On the Solutions for Contact Binary Systems
1987Although the pioneering paper of Lucy (1968) appeared already 18 years ago, the theory of contact binaries is by far not yet in a satisfactory state. This concerns in particular an aspect with which I will not deal here at all, namely the inability to reproduce theoretically the observed systems (light curves, period-colour relation).
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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 M Silva +2 more
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Contact angles of binary liquids and their interpretation
Journal of Adhesion Science and Technology, 1992A W Neumann
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Orbital Motion in the Vicinity of the Non-collinear Equilibrium Points of a Contact Binary Asteroid
Planetary and Space Science, 2015Jinglang Feng +2 more
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Changes in the orbital period of the near-contact binary BF Vir
Chinese Astronomy and Astrophysics, 2000Sheng-Bang Qian
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Evolutionary computations of the early-type contact binary SV Centauri
Astrophysics and Space Science, 1982Yasuhisa Nakamura
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