Fig. 2
The rotation curve from our galaxy with the dark-matter contribution, given by the sum of the triaxial pseudo-isothermal halo profile plus the two rings, which is determined from the EGRET excess of diffuse gamma rays (red data points).
International Journal of High-Energy Physics
The rotation curve from our galaxy with the dark-matter contribution, given by the sum of the triaxial pseudo-isothermal halo profile plus the two rings, which is determined from the EGRET excess of diffuse gamma rays (red data points).