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2016MNRAS.462.2706D - Mon. Not. R. Astron. Soc., 462, 2706-2714 (2016/November-1)
A method for evaluating models that use galaxy rotation curves to derive the density profiles.
DE ALMEIDA A.O.F., PIATTELLA O.F. and RODRIGUES D.C.
Abstract (from CDS):
Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): gravitation - galaxies: kinematics and dynamics - galaxies: spiral - dark matter - dark matter
Simbad objects: 6
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