Massive spectroscopic surveys of stars in the thick disk and halo populations of the Galaxy hold the potential to provide strong constraints on the processes involved in (and the timing of) the assembly history of the primary structural components of th
Context. Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fu...
textStudying massive star formation is hard, both observationally and theoretically. Many basic que...
Robust stellar age measurements, and the star formation histories (SFHs) they enable us to derive, a...
Massive spectroscopic surveys of stars in the thick disk and halo populations of the Galaxy hold the...
Dwarf spheroidal satellite galaxies have emerged a powerful probe of small-scale dark matter cluster...
Massive spectroscopic and imaging surveys of individual stars in the Milky Way are opening windows o...
We explore the motivation behind large stellar surveys in Galactic astronomy, in particular, surveys...
I If we are to develop a comprehensive and predictive theory of galaxy formation and evolution, it i...
The far outer regions of galactic disks allow an important probe of both star formation and galaxy f...
A local property of standard cosmology - growth of primordial perturbations - implies at least six d...
Resolved observations of nearby galaxies help us to understand the relationship between gas and star...
The archeological record of stars in the Milky Way opens a uniquely detailed window into the early f...
International audienceI review the recent instrumental progresses which allow to directly observe ga...
We investigate the physical properties of the progenitors of today living Milky Way-like galaxies th...
Within the Local Universe galaxies can be studied in great detail star by star. The Colour-Magnitude...
Context. Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fu...
textStudying massive star formation is hard, both observationally and theoretically. Many basic que...
Robust stellar age measurements, and the star formation histories (SFHs) they enable us to derive, a...
Massive spectroscopic surveys of stars in the thick disk and halo populations of the Galaxy hold the...
Dwarf spheroidal satellite galaxies have emerged a powerful probe of small-scale dark matter cluster...
Massive spectroscopic and imaging surveys of individual stars in the Milky Way are opening windows o...
We explore the motivation behind large stellar surveys in Galactic astronomy, in particular, surveys...
I If we are to develop a comprehensive and predictive theory of galaxy formation and evolution, it i...
The far outer regions of galactic disks allow an important probe of both star formation and galaxy f...
A local property of standard cosmology - growth of primordial perturbations - implies at least six d...
Resolved observations of nearby galaxies help us to understand the relationship between gas and star...
The archeological record of stars in the Milky Way opens a uniquely detailed window into the early f...
International audienceI review the recent instrumental progresses which allow to directly observe ga...
We investigate the physical properties of the progenitors of today living Milky Way-like galaxies th...
Within the Local Universe galaxies can be studied in great detail star by star. The Colour-Magnitude...
Context. Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fu...
textStudying massive star formation is hard, both observationally and theoretically. Many basic que...
Robust stellar age measurements, and the star formation histories (SFHs) they enable us to derive, a...
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