2009/05/11 by Noam I. Libeskind, Noam I Libeskind, Carlos S. Frenk +5
Physics and Astronomy · #Angular momentum #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Galaxy #Local Group #Milky Way #Momentum (technical analysis) #Satellite #Satellite galaxy #astro-ph.CO
paper · pdf · doi:10.1111/j.1365-2966.2009.15315.x
12 Pages, 10 Figures, Submitted to MNRAS
arxiv created 2009/05/11 · openalex publication_date 2009/09/02 · arxiv updated 2015/05/13 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The highly flattened distribution of satellite galaxies in the Milky Way (MW) presents a number of puzzles. First, its polar alignment stands out from the planar alignments commonly found in other galaxies. Secondly, recent proper-motion measurements reveal that the orbital angular momentum of at least three, and possibly as many as eight, of the MW's satellites points (within 30°) along the axis of their flattened configuration, suggesting some form of coherent motion. In this paper, we use a high-resolution cosmological simulation to investigate whether this pattern conflicts with the expectations of the cold dark matter model of structure formation. We find that this seemingly unlikely setup occurs often: approximately 35 per cent of the time, we find systems in which the angular momentum of three individual satellites points along, or close to, the short axis of the satellite distribution. In addition, in 30 per cent of the systems we find that the net angular momentum of the six best-aligned satellites lies within 35° of the short axis of the satellite distribution, as observed for the MW.