Implications of the Milky Way travel velocity for dynamical mass estimates of the Local Group
Katie Chamberlain (1, 2), Adrian M. Price-Whelan (2), Gurtina Besla, (1), Emily C. Cunningham (2), Nicol\'as Garavito-Camargo (2), Jorge, Pe\~narrubia (3), Michael S. Petersen (4) ((1) University of Arizona, (2), Flatiron Institute, (3) University of Edinburgh

TL;DR
This paper investigates how the measured travel velocity of the Milky Way affects the estimated total mass of the Local Group, revealing that accounting for this velocity reduces mass estimates by about 10-12%.
Contribution
It quantifies the impact of the Milky Way's travel velocity on Local Group mass estimates using recent kinematic data, highlighting the importance of non-equilibrium effects.
Findings
Incorporating the travel velocity lowers LG mass estimates by 10-12%.
More distant tracers could indicate even larger velocities, further decreasing mass estimates.
The travel velocity must be considered in future dynamical models of the Local Volume.
Abstract
The total mass of the Local Group (LG) is a fundamental quantity that enables interpreting the orbits of its constituent galaxies and placing the LG in a cosmological context. One of the few methods that allows inferring the total mass directly is the "Timing Argument," which models the relative orbit of the Milky Way (MW) and M31 in equilibrium. The MW itself is not in equilibrium, a byproduct of its merger history including the recent pericentric passage of the LMC, and recent work has found that the MW disk is moving with a lower bound "travel velocity" of with respect to the outer stellar halo. Previous Timing Argument measurements attempt to account for this non-equilibrium state, but have been restricted to theoretical predictions for the impact of the LMC specifically. In this paper, we quantify the impact of a travel velocity on recovered LG mass…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
