Figure 2 from Constraining Dark Matter Halo Profiles and Galaxy Formation Models Using Spiral Arm Morphology. II. Dark and Stellar Mass Concentrations for 13 Nearby Face-on Galaxies

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Constraining Dark Matter Halo Profiles and Galaxy Formation Models Using Spiral Arm Morphology. II. Dark and Stellar Mass Concentrations for 13 Nearby Face-on Galaxies

Authors: Marc S. Seigar, Benjamin L. Davis, Joel Berrier, and Daniel Kennefick

Seigar et al. 2014 The Astrophysical Journal 795 90.

Provider: AAS Journals

Caption: Figure 2.

Surface brightness profiles for 13 galaxies. The short-dashed line is the Sérsic fit to the bulge, the long-dashed line is the exponential disk fit, and the solid line is the total bulge+disk fit.

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