Pseudo Rotation Curve connecting the Galaxy, Dark Halo, and Local Group
Yoshiaki Sofue (Dept. Phys. Astroph, Kagoshima University, and Inst., Astronomy, Univ. Tokyo)

TL;DR
This paper constructs a combined rotation curve for the Galaxy and Local Group, revealing dark matter distribution and total mass estimates, and compares dark matter profiles with observational data.
Contribution
It introduces a method to connect Galactic and Local Group rotation curves, providing new insights into dark matter distribution and total mass estimates within the Local Group.
Findings
Dark matter in the Local Group is approximately 5 x 10^{12} solar masses.
The Galaxy's dark halo mass within 385 kpc is about 4 x 10^{11} solar masses.
The dark matter density transitions from Galactic to intracluster dominance around 100 kpc.
Abstract
We construct a Galacto-Local Group rotation curve, combining the Galactic rotation curve with a diagram, where galacto-centric radial velocities of outer globular clusters and member galaxies of the Local Group are plotted against their galacto-centric distances. The high-velocity ends of this pseudo rotation curve within a radius R ~ 150 kpc are well traced by a rotation curve calculated for the NFW (Navaro, Frenk, White) and Burkert dark halo models. The NFW model indicates that the Galaxy's mass within 385 kpc, half distance to M31, is ~ 4 x 10^{11}M_{sun}. High-velocity ends of the pseudo rotation curve for the entire Local Group up to 1.5 Mpc indicate isothermal nature with a terminal velocity of ~ 200 km/s. In order for the Local Group to be gravitationally bound, an order of magnitude larger mass than those of the Galaxy and M31 is required. This fact indicates that the Local…
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