The frozen outskirts: a cold Hubble flow and the mass of the Local Group
Danila Makarov, Dmitry Makarov, Lidia Makarova, Noam Libeskind

TL;DR
This study measures the total mass of the Local Group using the velocity field of peripheral galaxies, finding it confined within the virial radii of the Milky Way and Andromeda, with implications for local dynamics.
Contribution
It provides a new estimate of the Local Group's mass based on the cold Hubble flow, confirming mass confinement within the main galaxies' virial radii.
Findings
Local Group mass: (2.47 ± 0.15) × 10^{12} M_sun
Mass ratio of Milky Way to Andromeda: 0.74 ± 0.10
Galaxy velocity relative to barycenter: 62.6 ± 2.6 km/s
Abstract
We analyze the velocity field of peripheral members of the Local Group. The Hubble flow at distances from 400 to 1400~kpc, formed by 7 of 11 nearby galaxies, is characterized by an extremely small line-of-sight velocity dispersion of 15 km/s, which differs significantly from the predictions of cosmological simulations of about 70 km/s. This fact allows us to determine the total mass of the Local Group as using an analytical model of the Hubble flow around a spherical overdensity in the standard flat \LCDM{} universe. The practical equality of this mass to the sum of the masses of our Galaxy and the Andromeda Galaxy, as well as the absence of mass growth in the range of distances under consideration, gives grounds to conclude that the entire mass of the Local Group is confined within the virial radii around its two main galaxies. The…
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