High-resolution rotation curves of low surface brightness galaxies

Jan, 2002
Published in:
  • Astron.Astrophys. 385 (2002) 816
e-Print:

Citations per year

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Abstract: (arXiv)
We present high-resolution rotation curves of a sample of 26 low surface brightness galaxies. From these curves we derive mass distributions using a variety of assumptions for the stellar mass-to-light ratio. We show that the predictions of current Cold Dark Matter models for the density profiles of dark matter halos are inconsistent with the observed curves. The latter indicate a core-dominated structure, rather than the theoretically preferred cuspy structure.
  • GALAXIES STRUCTURE
  • GALAXIES KINEMATICS
  • GALAXIES DYNAMICS
  • GALAXIES HALOS
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