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

Astronomy and Astrophysics – Astrophysics

Scientific paper

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accepted by A&A, 5 pages

Scientific paper

10.1051/0004-6361:20041122

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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