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P. François, G. Cescutti, P. Bonifacio, E. Caffau, L. Monaco, M. Steffen, J. Puschnig, F. Calura, S. Cristallo, P. Di Marcantonio, V. Dobrovolskas, M. Franchini, A. J. Gallagher, C. J. Hansen, A. Korn, A. Kučinskas, R. Lallement, L. Lombardo, F. Lucertini, L. Magrini, A. M. Matas Pinto, F. Matteucci, A. Mucciarelli, L. Sbordone, M. Spite, et al. Astronomy & Astrophysics 686 A295 (2024) https://doi.org/10.1051/0004-6361/202449539
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The stellar halo in Local Group Hestia simulations
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Stellar halo striations from assumptions of axisymmetry
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The stellar halo in Local Group Hestia simulations
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The Global Dynamical Atlas of the Milky Way Mergers: Constraints from Gaia EDR3–based Orbits of Globular Clusters, Stellar Streams, and Satellite Galaxies
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Gastro Library. I. The Simulated Chemodynamical Properties of Several Gaia–Sausage–Enceladus-like Stellar Halos
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The GALAH Survey: No Chemical Evidence of an Extragalactic Origin for the Nyx Stream
Daniel B. Zucker, Jeffrey D. Simpson, Sarah L. Martell, Geraint F. Lewis, Andrew R. Casey, Yuan-Sen 源森 Ting 丁, Jonathan Horner, Thomas Nordlander, Rosemary F. G. Wyse, Tomaž Zwitter, Joss Bland-Hawthorn, Sven Buder, Martin Asplund, Gayandhi M. De Silva, Valentina D’Orazi, Ken C. Freeman, Michael R. Hayden, Janez Kos, Jane Lin, Karin Lind, Katharine J. Schlesinger, Sanjib Sharma and Dennis Stello The Astrophysical Journal Letters 912(2) L30 (2021) https://doi.org/10.3847/2041-8213/abf7cd
Constraints on the Assembly History of the Milky Way's Smooth, Diffuse Stellar Halo from the Metallicity-dependent, Radially Dominated Velocity Anisotropy Profiles Probed with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia
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VINTERGATAN – II. The history of the Milky Way told by its mergers
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Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances*
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G 112-43/44: A metal-poor binary star with a unique chemical composition and Helmi stream kinematics
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Streams, Substructures, and the Early History of the Milky Way
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Reviving old controversies: is the early Galaxy flat or round?
Evidence from the H3 Survey That the Stellar Halo Is Entirely Comprised of Substructure
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Evidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy
Danny Horta, Ricardo P Schiavon, J Ted Mackereth, et al. Monthly Notices of the Royal Astronomical Society 500(1) 1385 (2020) https://doi.org/10.1093/mnras/staa2987
The metal-rich halo tail extended in |z|: a characterization with Gaia DR2 and APOGEE
Emma Fernández-Alvar, José G Fernández-Trincado, Edmundo Moreno, et al. Monthly Notices of the Royal Astronomical Society 487(1) 1462 (2019) https://doi.org/10.1093/mnras/stz1299
The Milky Way has no in-situ halo other than the heated thick disc
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The shape of the Galactic halo withGaiaDR2 RR Lyrae. Anatomy of an ancient major merger
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Mergers, tidal interactions, and mass exchange in a population of disc globular clusters
StarGO: A New Method to Identify the Galactic Origins of Halo Stars
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Kinematics of Highly r-process-enhanced Field Stars: Evidence for an Accretion Origin and Detection of Several Groups from Disrupted Satellites