Fig. 17 from Mass Models for Low Surface Brightness Galaxies with High‐Resolution Optical Velocity Fields

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Mass Models for Low Surface Brightness Galaxies with High‐Resolution Optical Velocity Fields

Authors: Rachel Kuzio de Naray, Stacy S. McGaugh, and W. J. G. de Blok

Kuzio de Naray, McGaugh, & de Blok 2008 The Astrophysical Journal 676 920.

Provider: AAS Journals

Caption: Fig. 17.

Required noncircular motions, assuming an isotropic dispersion, to reconcile the difference between the NFWconstr velocity and the observed dark matter velocity. Line types are as in Fig. 16.

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