Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations

Abstract

We use the recently proposed scale-free mass estimators to determine the masses of the Milky Way (MW) and Andromeda (M31) galaxy in a dark matter only Constrained Local UniversE Simulation (CLUES). While these mass estimators work rather well for isolated spherical host systems, we examine here their applicability to a simulated binary system with a unique satellite population similar to the observed satellites of MW and M31. We confirm that the scale-free estimators work also very well in our simulated Local Group galaxies with the right number of satellites which follow the observed radial distribution. In the isotropic case and under the assumption that the satellites are tracking the total gravitating mass, the power-law index of the radial satellite distribution $N(<r)\propto r^{3-\gamma }$ is directly related to the host's mass profile $M(<r)\propto r^{1-\alpha }$ as $\alpha =\gamma -2$. The use of this relation for any given $\gamma$ leads to highly accurate mass estimations which is a crucial point for observer, since they do not know a priori the mass profile of the MW and M31 haloes. We discuss possible bias in the mass estimators and conclude that the scale-free mass estimators can be satisfactorily applied to the real MW and M31 system.

14 pages, 6 figures, 6 tables. Accepted in MNRAS 2012 March 29. Received 2012 March 29; in original form 2011 September 29

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Cited by in corpus (14)

• The Space Motion of Leo I: The Mass of the Milky Way's Dark Matter Halo
• A distance of 13 Mpc resolves the claimed anomalies of the galaxy lacking dark matter
• Dwarf Galaxies and the Cosmic Web
• The Hestia project: simulations of the Local Group
• The outer halo globular cluster system of M31 - II. Kinematics
• The Imprint of Reionization on the Star Formation Histories of Dwarf Galaxies
• Mergers and the outside-in formation of dwarf spheroidals
• The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile
• The mass of our Galaxy from satellite proper motions in the Gaia era
• The SLUGGS Survey: The mass distribution in early-type galaxies within five effective radii and beyond
• Dark Matter in the Local Universe
• Cold versus Warm Dark Matter simulations of a galaxy group
• The Proper Motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy