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The constant density region of the dark halos of spiral galaxies

Paolo Salucci
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Abstract

From the kinematics of 137 spirals we find that the DM halo density profiles are self-similar at least out to R_opt and show core radii much larger that the corresponding disk scale-lenghts. The luminous regions of spirals consist of stellar disks embedded in dark halos with roughly constant density. With respect to previous work, the present evidence is obtained by means of a robust method and for a large and complete sample of normal spirals.

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Paolo Salucci. 2000-07-26. The constant density region of the dark halos of spiral galaxies. https://doi.org/10.1046/j.1365-8711.2001.04076.x

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