| Issue |
EAS Publications Series
Volume 20, 2006
Mass Profiles and Shapes of Cosmological Structures
|
|
|---|---|---|
| Page(s) | 277 - 278 | |
| DOI | https://doi.org/10.1051/eas:2006088 | |
| Published online | 19 May 2006 | |
Mass Profiles and Shapes of Cosmological Structures
G.A. Mamon, F. Combes, C. Deffayet and B. Fort (eds)
EAS Publications Series, 20 (2006) 277-278
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
1
Theoretical Physics, University of Oxford, 1
Keble Road, Oxford OX1
3NP, UK
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