Galactic orbital motions in the Dark Matter, MOdified Newtonian Dynamics and MOdified Gravity scenarios
arXiv:0904.0219 · doi:10.1111/j.1365-2966.2009.15811.x
Abstract
We simultaneously integrate in a numerical way the equations of motion of both the Magellanic Clouds (MCs) in MOND, MOG and CDM for -1 <= t <= +1 Gyr to see if, at least in principle, it is possible to discriminate between them (Abridged version).
LaTex2e, 11 pages, 2 tables, 8 figures. Issues concerning the masses of MCs clarified. Integration time changed to -1 Gyr <= t <= +1 Gyr. To appear in Monthly Notices of the Royal Astronomical Society (MNRAS)