We present Halpha rotation curves for a sample of 15 dwarf and LSB galaxies. From these, we derive limits on the slopes of the central mass distributions. Assuming the density distributions of dark matter halos follow a power-law at small radii, rho(r)~r^(-alpha), we find inner slopes in the range 0
CITATION STYLE
Swaters, R. A., Madore, B. F., van den Bosch, F. C., & Balcells, M. (2003). The Central Mass Distribution in Dwarf and Low Surface Brightness Galaxies. The Astrophysical Journal, 583(2), 732–751. https://doi.org/10.1086/345426
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