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The Local Group’s mass: probably no more than the sum of its parts

Sawala, Till; Teeriaho, Meri; Johansson, Peter H

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Authors

Meri Teeriaho

Peter H Johansson



Abstract

The total mass of the Local Group and the masses of its primary constituents, the Milky Way (MW) and M31, are important anchors for several cosmological questions. Recent independent measurements have consistently yielded halo masses close to 1012M for the MW, and 1–2 × 1012M for M31, while estimates derived from the pair’s kinematics via the ‘timing argument’ have yielded a combined mass of around 5 × 1012M. We analyse the extremely large UCHUU simulation to constrain the mass of the Local Group and its two most massive members. First, we demonstrate the importance of selecting pairs whose kinematics reflect their mutual interactions. Adopting the observed separation and radial velocity, we obtain a weighted posterior of 75+65 −40 km s−1 for the uncertain transverse velocity. Via Gaussian process regression, we infer a total mass of 3.2+1.2 −0.9 × 1012M, significantly below the timing argument value. Importantly, the remaining uncertainty is not rooted in the analysis or observational errors, but in the irreducible scatter in the kinematics–mass relation. We further find a mass for the less massive halo of 0.9+0.6 −0.3 × 1012M and for the more massive halo of 2.3+1.0 −0.9 × 1012M, consistent with independent measurements of the masses of MW and M31, respectively. Incorporating the MW mass as an additional prior let us constrain
all measurements further and determine that the MW is very likely less massive than M31.

Citation

Sawala, T., Teeriaho, M., & Johansson, P. H. (2023). The Local Group’s mass: probably no more than the sum of its parts. Monthly Notices of the Royal Astronomical Society, 521(4), 4863-4877. https://doi.org/10.1093/mnras/stad883

Journal Article Type Article
Acceptance Date Mar 17, 2023
Online Publication Date Mar 22, 2023
Publication Date 2023-06
Deposit Date Jan 2, 2024
Publicly Available Date Jan 2, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 521
Issue 4
Pages 4863-4877
DOI https://doi.org/10.1093/mnras/stad883
Public URL https://durham-repository.worktribe.com/output/2078321

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