Fig. 5 from Accurate Determination of the Mass Distribution in Spiral Galaxies. II. Testing the Shape of Dark Halos

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Accurate Determination of the Mass Distribution in Spiral Galaxies. II. Testing the Shape of Dark Halos

Authors: Sébastien Blais-Ouellette, Philippe Amram, and Claude Carignan

Blais‐Ouellette, Amram, & Carignan 2001 The Astronomical Journal 121 1952.

Provider: AAS Journals

Caption: Fig. 5.

Density profiles of the four models: pseudoisothermal sphere (solid line), KKBP (dotted line), Burkert (long‐dashed line), and NFW (short‐dashed line).

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