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arXiv · 0804.2476

On the structure of tidal tails

Andreas H. W. Küpper·Andrew Macleod·Douglas C. Heggie
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Abstract

We examine the longitudinal distribution of the stars escaping from a cluster along tidal tails. Using both theory and simulations, we show that, even in the case of a star cluster in a circular galactic orbit, when the tide is steady, the distribution exhibits maxima at a distance of many tidal radii from the cluster.

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Andreas H. W. Küpper, Andrew Macleod, Douglas C. Heggie. 2008-04-15. On the structure of tidal tails. https://doi.org/10.1111/j.1365-2966.2008.13323.x

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