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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.CORE PARAMETERS OF DM HALOS
- 2.1.Rotation Curve
Decomposition. I. Technique
- 2.2.Rotation Curve
Decomposition. II. Our Assumptions
- 2.3.Rotation Curve
Decomposition. III. Galaxy Selection Criteria
- 2.4.Matching Pseudo-Isothermal Models
to the Isothermal Sphere
- 2.5.Central Densities of Dwarf
Spheroidal and Irregular Galaxies
- 3.DM HALO SCALING LAWS
- 4.CONCLUSIONS
- REFERENCES