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Stellar populations and dynamics in the Milky Way galaxy

2001
Our Galaxy offers a unique opportunity to deduce the important physics involved in galaxy formation from observations of those old stars that were formed at the time of the formation of the Milky Way, and whose present properties contain some fossil record of the Galaxy’s history.
openaire   +1 more source

Mapping the tilt of the Milky Way bulge velocity ellipsoids with ARGOS and Gaia DR2

Monthly Notices of the Royal Astronomical Society, 2021
Juntai Shen   +2 more
exaly  

Vertical Structure of the Milky Way Disk with Gaia DR3

Galaxies, 2023
Katherine Vieira   +2 more
exaly  

Dynamical effects of satellite accretion on the Milky Way

ΛCDM cosmology predicts that galaxies grow through the process of hierarchical structure formation. In the Milky Way (MW) galaxy, evidence of satellite accretion is present through observations of stellar streams in the outer halo, and chemo-kinematically distinct stellar populations in the inner regions. Recent surveys of the MW stars such as Gaia and
openaire   +2 more sources

Testing gravity with the Milky Way: Yukawa potential

Physical Review D, 2021
Luca Amendola   +2 more
exaly  

The mass of our Milky Way

Science China: Physics, Mechanics and Astronomy, 2020
Zhaozhou Li   +2 more
exaly  

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