Stellar halo streams in the Solar neighbourhood
Rainer J. Klement (MPIA Heidelberg)

TL;DR
This paper reviews the discovery and analysis of stellar halo streams in the Solar neighborhood, emphasizing how phase-space data reveals the Galaxy's hierarchical formation history and the importance of upcoming Gaia data for future research.
Contribution
It provides a comprehensive overview of the current state of stellar halo stream research and discusses strategies for identifying these structures in the Milky Way.
Findings
Large-scale surveys have revealed thousands of halo stars with full phase-space data.
Stellar streams retain chemical and kinematic signatures of their origins.
Future Gaia data will enable more precise disentangling of Galactic building blocks.
Abstract
The phase-space structure of our Galaxy holds the key to understand and reconstruct its formation. The Lambda-CDM model predicts a richly structured phase-space distribution of dark matter and (halo) stars, consisting of streams of particles torn from their progenitors during the process of hierarchical merging. While such streams quickly loose their spatial coherence in the process of phase mixing, the individual stars keep their common origin imprinted into their kinematic and chemical properties, allowing the recovery of the Galaxy's individual "building blocks". The field of Galactic Archeology has witnessed a dramatic boost over the last decade, thanks to the increasing quality and size of available data sets. This is especially true for the solar neighborhood, a volume of 1-2 kpc around the sun, where large scale surveys like SDSS/SEGUE continue to reveal the full 6D phase-space…
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