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arXiv · astro-ph/0410421

The great disk of Milky-Way satellites and cosmological sub-structures

Pavel Kroupa·Christian Theis·Christian M. Boily
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Abstract

We show that the shape of the observed distribution of Milky Way (MW) satellites is inconsistent with being drawn from a cosmological sub-structure population with a confidence of 99.5 per cent. Most of the MW satellites therefore cannot be related to dark-matter dominated satellites.

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Pavel Kroupa, Christian Theis, Christian M. Boily. 2004-10-18. The great disk of Milky-Way satellites and cosmological sub-structures. https://doi.org/10.1051/0004-6361%3A20041122

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