The kinematics of the most metal-poor stars provide a window into the early formation and accretion history of the Milky Way (MW). Here, we use five high-resolution cosmological zoom-in simulations (similar to 5 x 10(6) star particles) of MW-like galaxies taken from the NIHAO-UHD project, to investigate the origin of low-metallicity stars ([Fe/H]</p
We explore the predictions of the standard hierarchical clustering scenario of galaxy formation, reg...
By means of high-resolution cosmological hydrodynamical simulations of Milky Way (MW) like disc gala...
Here we investigate the evolution of a MilkyWay (MW)-like galaxy with the aim of predicting the prop...
The kinematics of the most metal-poor stars provide a window into the early formation and accretion ...
Low-metallicity stars give rise to unique spectacular transients and are of immense interest for und...
We use Gaia DR2 astrometric and photometric data, published radial velocities and MESA models to inf...
We investigate the metallicity distribution function (MDF) of the Galactic halo and the relative fra...
We explore the predictions of the standard hierarchical clustering scenario of galaxy formation, reg...
By means of high-resolution cosmological hydrodynamical simulations of Milky Way (MW) like disc gala...
Here we investigate the evolution of a MilkyWay (MW)-like galaxy with the aim of predicting the prop...
The kinematics of the most metal-poor stars provide a window into the early formation and accretion ...
Low-metallicity stars give rise to unique spectacular transients and are of immense interest for und...
We use Gaia DR2 astrometric and photometric data, published radial velocities and MESA models to inf...
We investigate the metallicity distribution function (MDF) of the Galactic halo and the relative fra...
We explore the predictions of the standard hierarchical clustering scenario of galaxy formation, reg...
By means of high-resolution cosmological hydrodynamical simulations of Milky Way (MW) like disc gala...
Here we investigate the evolution of a MilkyWay (MW)-like galaxy with the aim of predicting the prop...