EAS Publications Series
Volume 20, 2006Mass Profiles and Shapes of Cosmological Structures
|Page(s)||277 - 278|
|Published online||19 May 2006|
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 277-278
Testing the MOND formula in the Galaxy
Theoretical Physics, University of Oxford, 1
Keble Road, Oxford OX1
2 Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Belgium
The inner Galaxy is completely dominated by baryons, contrary to the predictions of CDM cosmology, whilst the observations are compatible with MOND if the local circular speed is smaller than 220 km s-1 and the asymptotic circular velocity close to 170 km s-1.
© EAS, EDP Sciences, 2006
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