Dwarf Galaxies and Star Clusters in Tidal Tails

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We summarize the properties of tidal dwarf candidates in a sample of interacting galaxies and classify objects in tidal tails depending on their morphological appearance. New high-resolution dynamical models are needed to understand how the different structures seen in tidal tails are formed.
5 pages, to be published in "Extragalactic Star Clusters", eds. E.K. Grebel, D. Geisler, D. Minniti, IAU Symposium Series Vol. 207

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/3040

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0107194
 http://arxiv.org/abs/astro-ph/0107194

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arXiv