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2021ApJ...920L..10L - Astrophys. J., 920, L10-L10 (2021/October-2)
Galaxy rotation curves disfavor traditional and self-interacting dark matter halos, preferring a disk component or Einasto function.
LOIZEAU N. and FARRAR G.R.
Abstract (from CDS):
Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.
Journal keyword(s): Baryonic dark matter - Dark matter - Galaxy rotation curves - Galaxy dynamics - Galaxy physics
Simbad objects: 11
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