We present spectra of six metal-poor stars in two of the ultra-faint dwarf galaxies orbiting the Milky Way (MW), Ursa Major II, and Coma Berenices obtained with the Keck/High Resolution Echelle Spectrometer (HIRES). These observations include the first high-resolution spectroscopic observations of extremely metal-poor ([Fe/H] -2.5) of the MW halo, but they also suggest that the faintest known dwarfs may be the primary contributors to the metal-poor end of the MW halo metallicity distribution.Astronom
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
We present a detailed abundance analysis based on high-resolution and high signal-to-noise spectra o...
We present a comprehensive abundance analysis of 20 elements for 16 new low-metallicity stars from t...
We present spectra of six metal-poor stars in two of the ultra-faint dwarf galaxies orbiting the Mil...
High resolution spectroscopy of stars belonging to two extremely low luminosity dwarf galaxies. Stud...
We present new metallicity measurements for 298 individual red giant branch stars in eight of the le...
The most metal-poor stars in dwarf spheroidal galaxies (dSphs) can show the nucleosynthetic patterns...
The SkyMapper Southern Sky Survey is carrying out a search for the most metal-poor stars in the Gala...
We present high-resolution Magellan/MIKE spectroscopy of the brightest star in the ultra-faint dwarf...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
Context. Individual stars in dwarf spheroidal galaxies around the Milky Way Galaxy have been studied...
We present new metallicity measurements for 298 individual red giant branch stars in eight of the le...
Unevolved metal poor stars are the witness of the early evolution of the Galaxy. The determination o...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the G...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
We present a detailed abundance analysis based on high-resolution and high signal-to-noise spectra o...
We present a comprehensive abundance analysis of 20 elements for 16 new low-metallicity stars from t...
We present spectra of six metal-poor stars in two of the ultra-faint dwarf galaxies orbiting the Mil...
High resolution spectroscopy of stars belonging to two extremely low luminosity dwarf galaxies. Stud...
We present new metallicity measurements for 298 individual red giant branch stars in eight of the le...
The most metal-poor stars in dwarf spheroidal galaxies (dSphs) can show the nucleosynthetic patterns...
The SkyMapper Southern Sky Survey is carrying out a search for the most metal-poor stars in the Gala...
We present high-resolution Magellan/MIKE spectroscopy of the brightest star in the ultra-faint dwarf...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
Context. Individual stars in dwarf spheroidal galaxies around the Milky Way Galaxy have been studied...
We present new metallicity measurements for 298 individual red giant branch stars in eight of the le...
Unevolved metal poor stars are the witness of the early evolution of the Galaxy. The determination o...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
Context. The most metal-poor stars in the Milky Way witnessed the early phases of formation of the G...
We present a homogeneous chemical abundance analysis of 16 elements in 190 metal-poor Galactic halo ...
We present a detailed abundance analysis based on high-resolution and high signal-to-noise spectra o...
We present a comprehensive abundance analysis of 20 elements for 16 new low-metallicity stars from t...