Fig. 11 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. 11.

Isothermal and NFW halo fits for NGC 4395. Line types are as in Fig. 5. The solid magenta line in the maximum disk NFW plot is the total baryonic rotation curve. See text for details.

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