Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-30872
Klimentowski, J; Lokas, E L; Kazantzidis, S; Mayer, L; Mamon, G A (2009). Tidal evolution of discy dwarf galaxies in the Milky Way potential: the formation of dwarf spheroidals. Monthly Notices of the Royal Astronomical Society, 397(4):2015-2029.
PDF (Accepted manuscript, Version 2)
PDF (Accepted manuscript, Version 1)
We conduct high-resolution collisionless N-body simulations to investigate the tidal evolution of dwarf galaxies on an eccentric orbit in the Milky Way (MW) potential. The dwarfs originally consist of a low surface brightness stellar disc embedded in a cosmologically motivated dark matter halo. During 10 Gyr of dynamical evolution and after five pericentre passages, the dwarfs suffer substantial mass loss and their stellar component undergoes a major morphological transformation from a disc to a bar and finally to a spheroid. The bar is preserved for most of the time as the angular momentum is transferred outside the galaxy. A dwarf spheroidal (dSph) galaxy is formed via gradual shortening of the bar. This work thus provides a comprehensive quantitative explanation of a potentially crucial morphological transformation mechanism for dwarf galaxies that operates in groups as well as in clusters. We compare three cases with different initial inclinations of the disc and find that the evolution is fastest when the disc is coplanar with the orbit. Despite the strong tidal perturbations and mass loss, the dwarfs remain dark matter dominated. For most of the time, the one-dimensional stellar velocity dispersion, σ, follows the maximum circular velocity, Vmax, and they are both good tracers of the bound mass. Specifically, we find that M_ V_^ and V_ in agreement with earlier studies based on pure dark matter simulations. The latter relation is based on directly measuring the stellar kinematics of the simulated dwarf, and may thus be reliably used to map the observed stellar velocity dispersions of dSphs to halo circular velocities when addressing the missing satellites problem.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Uncontrolled Keywords:||galaxies: dwarf; galaxies: fundamental parameters; galaxies: kinematics and dynamics; Local Group; cosmology: dark matter|
|Deposited On:||26 Feb 2010 14:10|
|Last Modified:||27 Nov 2013 19:40|
|Funders:||Polish Ministry of Science and Higher Education [N N203 0253 33] , CNRS/PAN|
|Additional Information:||The attached file is a preprint (accepted version) of an article published in Monthly Notices of the Royal Astronomical Society. The definitive version is available at www3.interscience.wiley.com|
|Citations:||Web of Science®. Times Cited: 39|
Scopus®. Citation Count: 38
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