The Great disk of Milky Way satellites and cosmological sub-structures
Oct, 2004
5 pages
Published in:
- Astron.Astrophys. 431 (2005) 517-521
e-Print:
- astro-ph/0410421 [astro-ph]
View in:
Citations per year
Abstract: (arXiv)
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.- COSMOLOGY
- GALAXY EVOLUTION
- GALAXY HALO
- DWARF GALAXIES
- GALAXIES KINEMATICS
- GALAXIES DYNAMICS
- LOCAL GROUP
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