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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