2025/03/16 by Danila Makarov, Dmitry Makarov, Kirill Kozyrev +1 · 1 voice
Physics and Astronomy · #astro-ph.GA
paper · pdf · doi:10.3390/universe11050144
arxiv published 2025/03/16 · arxiv updated 2025/04/30
The total mass of a galaxy group, such as the Milky Way (MW) and the Andromeda Galaxy (M 31), is typically determined from the kinematics of satellites within their virial zones. Bahcall and Tremaine (1981) proposed the v2r estimator as an alternative to the virial theorem. In this work, we extend their approach by incorporating the three-dimensional spatial distribution of satellites within the system to improve the reliability and accuracy of galaxy mass estimates. Applying this method to a comprehensive dataset of Local Group satellites based on recent, high-precision distance measurements, we estimate the total mass of the MW to be (7.9 ± 2.3) × 1011 M_\odot and that of M~31 to be (15.5 ± 3.4) × 1011 M_\odot. The effectiveness of the method is constrained by the precision of distance measurements, making it particularly well suited for the Local Group, but challenging to apply to more distant systems.