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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 6.

Spiral arm pitch angle vs. NFW concentration. The open triangle represents Malin 1 (Seigar 2008), the star represents M31 (Seigar et al. 2008a), the open circle represents M33 (Seigar 2011), and the filled squares represent the current sample.

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