Fig. 4 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. 4.

Halo fits to the DensePak rotation curves. The red solid line represents the best‐fit isothermal halo, the green short‐dashed line represents the best‐fit unconstrained NFW halo, and the black long‐dashed line represents the best‐fit NFW_constr halo. NFW_constr fits were only made to UGC 4325, DDO 64, and F583‐1.

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