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Amina Helmi
The Tilt of the Velocity Ellipsoid in the Milky Way with Gaia DR2 Jorrit H
Observational Aspects of Globular Cluster and Halo Stars in the GALAH Survey
New Perspectives in Understanding the Galactic Halo
Elemental Abundances in the Local Group: Tracing the Formation History of the Great Andromeda Galaxy
Mass and Shape of the Milky Way's Dark Matter Halo with Globular
Curriculum Vitae of Prof. Dr. Amina Helmi
THE ONCE and FUTURE MILKY WAY Data from the Gaia Spacecraft Are Radically Transforming How We See the Evolution of Our Galaxy
Halo Streams As Relicts from the Formation of the Milky Way 3 Consist of 300 – 500 Stellar Streams with Internal Velocity Dispersions of ∼ 5 Km S−1
Chemo-Dynamical Simulations of the Milky Way
Amina Helmi; Star of the Milky
A Box Full of Chocolates: the Rich Structure of the Nearby Stellar Halo Revealed by Gaia and RAVE Amina Helmi1, Jovan Veljanoski1, Maarten A
→ the BILLION STAR SURVEYOR GAIA DATA RELEASE 2 Media Kit
Voyage 2050 Final Recommenda�Ons from the Voyage 2050 Senior Commi�Ee
Chapter 4 the Bar and the Large Scale Velocity Gradients in the Galactic Disk
Research Assessment 2010-‐2015 March 2017
Robyn E. Sanderson MC 350-17, 1200 E
Amina Helmi, the “Archeologist of the Milky Way,” Explains How Our Own Galaxy Could Unlock the Mystery of Dark Matter
Unravelling the Origins of the Milky Way with Gaia
Top View
Streams, Substructures and the Early History of the Milky Way Arxiv
Call for Membership of Topical Teams for the Voyage 2050 Long-Term Plan in the ESA Science Programme