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- W1651174725 abstract "A simple and natural explanation for the dynamics and morphology of the Local Group Dwarf Spheroidal galaxies, Draco (Dra) and Ursa Minor (UMi), is that they are weakly unbound stellar systems with no significant dark matter component. A gentle, but persistent, Milky Way (MW) tide has left them in their current kinematic and morphological state (the “parametric tidal excitation”). A new test of a dark matter dominated dS potential follows from a careful observation of the “clumpiness” of the dS stellar surface density." @default.
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- W1651174725 date "2004-01-01" @default.
- W1651174725 modified "2023-09-26" @default.
- W1651174725 title "Evidence for Light-weight Local Group Dwarf Spheroidal Galaxies" @default.
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- W1651174725 doi "https://doi.org/10.1017/s0074180900183652" @default.
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