On the Distribution of Orbital Poles of Milky Way Satellites

Christopher Palma; Steven R. Majewski; Kathryn V. Johnston

doi:10.1086/324137

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arXiv · astro-ph/0108474

On the Distribution of Orbital Poles of Milky Way Satellites

Christopher Palma·Steven R. Majewski·Kathryn V. Johnston

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Abstract

In numerous studies of the outer Galactic halo some evidence for accretion has been found. If the outer halo did form in part or wholly through merger events, we might expect to find coherent streams of stars and globular clusters following similar orbits as their parent objects, which are assumed to be present or former Milky Way dwarf satellite galaxies. We present a study of this phenomenon by assessing the likelihood of potential descendant ``dynamical families'' in the outer halo. We conduct two analyses: one that involves a statistical analysis of the spatial distribution of all known Galactic dwarf satellite galaxies (DSGs) and globular clusters, and a second, more specific analysis of those globular clusters and DSGs for which full phase space dynamical data exist. In both cases our methodology is appropriate only to members of descendant dynamical families that retain nearly aligned orbital poles today. Since the Sagittarius dwarf (Sgr) is considered a paradigm for the type of merger/tidal interaction event for which we are searching, we also undertake a case study of the Sgr system and identify several globular clusters that may be members of its extended dynamical family. (ABRIDGED)

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Christopher Palma, Steven R. Majewski, Kathryn V. Johnston. 2001-08-29. On the Distribution of Orbital Poles of Milky Way Satellites. https://doi.org/10.1086/324137

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