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- W3148503721 abstract "Some dwarf galaxies have HI rotation curves that are completely dominated by a surrounding dark matter (DM) halo (e.g. Carignan & Freeman 1988). These objects represent ideal candidates for an investigation of the density structure of low-mass DM halos as the uncertainties resulting from the subtraction of the visible component are small, even in the innermost regions. Flores & Primack (1994) and Moore (1994) compared the observed DM rotation curves with the profiles, predicted from cosmological cold dark matter (CDM) calculations. They found an interesting discrepancy: whereas the calculations lead to a DM density distribution which diverges as ρ ∼ r −1 in the inner parts, the observed rotation curves indicate shallow DM cores which can be described by an isothermal density profile with finite central density." @default.
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- W3148503721 date "1996-01-01" @default.
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- W3148503721 title "The Structure of Dark Matter Halos in Dwarf Galaxies" @default.
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- W3148503721 doi "https://doi.org/10.1017/s0074180900232324" @default.
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