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Effects of Mean and Tidal Current Interaction on the Tidally Induced Residual Current

Journal of Physical Oceanography, 1987
Abstract A weakly nonlinear depth-dependent tidal model has been developed to study the effects of mean and tidal current interaction on the tidally induced residual current. The model is applied to the northern and southern sides of Georges Bank. The weakly nonlinear approximation is reasonable for the southern section, but only marginally applicable ...
Yuxiang Tang, Kim-Tai Tee
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Tidal interactions and the merging of galaxies

Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1980
Abstract Interpenetrating encounters between galaxies may occur frequently in groups and clusters of galaxies, and will be particularly common if most galaxies possess extended massive halos. When the encounter velocity of two galaxies is comparable with the velocity dispersion of the stars they contain, collisions are highly ...
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Tidal Phenomena in Interacting Galaxies

1990
We present evidence for the action of tidal stripping and tidal friction in interacting binary galaxies. This evidence comes from the morphological distortions seen in pairs of elliptical galaxies, and from the kinematic peculiarities seen both in elliptical galaxy rotation curves and in spiral galaxy HI 21cm profiles.
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Tidal interactions between galaxies

2005
The basic properties of galaxies and simple models of their formation are discussed and different types of interaction between galaxies are described. The dynamics of galactic interactions, statistical approaches and model calculations are reviewed and the significance of interactions in the evolution of galaxies is presented.
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Tidal Features in Interacting Galaxies

2013
We use OSIRIS in its long-slit mode to look for mass transfer and induced star formation in the interacting galaxy pair KPG 468.
Fuentes-Carrera, Isaura   +6 more
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Tidal interactions and the massive halo hypothesis

Nature, 1977
THE idea that galaxies may be surrounded by large amounts of unseen material has become very popular. The arguments favouring such massive haloes are almost all based on the dynamical analysis of galaxies either individually or in groups, and they have been cogently assembled by Einasto et al.1 and by Ostriker et al.2.
SIMON D. M. WHITE, NIGEL A. SHARP
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Generalized Gordon decomposition and the tidal interaction

Physical Review D, 1977
A generalized form of the Gordon decomposition technique is applied to the Dirac spin density. It is shown that this technique makes explicit the geodesic deviation and consequently the tidal force implied by the linearized coupling of the spin density to the gauge field associated with minimal gravitational coupling.
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Tidal interactions of disc galaxies

Monthly Notices of the Royal Astronomical Society, 1982
P. L. Palmer, J. Papaloizou
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