arXiv · astro-ph/0201276
H alpha rotation curves of Low Surface Brightness galaxies
Abstract
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.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
W. J. G. de Blok, A. Bosma. 2002-01-16. H alpha rotation curves of Low Surface Brightness galaxies. https://doi.org/10.1051/0004-6361%3A20020080
Cite the original work for its findings. Save a collection to share your selection of sources.