We report the discovery of the Little Cub, an extremely metal-poor star-forming galaxy in the local universe, found in the constellation Ursa Major (a.k.a. the Great Bear). We first identified the Little Cub as a candidate metal-poor galaxy based on its Sloan Digital Sky Survey photometric colors, combined with spectroscopy using the Kast spectrograph on the Shane 3 m telescope at Lick Observatory. In this Letter, we present high-quality spectroscopic data taken with the Low Resolution Imaging Spectrometer at Keck Observatory, which confirm the extremely metal-poor nature of this galaxy. Based on the weak [O III] λ4363 Å emission line, we estimate a direct oxygen abundance of 12 + log(O/H) = 7.13 ± 0.08, making the Little Cub one of t...
Metal-poor stars in the Milky Way are local relics of the epoch of the first stars and the first gal...
Early-type dwarfs (ETDs) are the end points of the evolution of low-mass galaxies whose gas supply h...
We present new Keck/HIRES data of the most metal-poor damped Lyman-alpha (DLA) system currently know...
We report a method of identifying candidate low-metallicity blue compact dwarf galaxies (BCDs) from ...
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 report two new low-metallicity blue compact dwarf galaxies (BCDs), WISEP J080103.93+264053.9 (her...
In this paper we analyze the kinematics, chemistry, and physical properties of a sample of the most ...
© 2021. The American Astronomical Society. All rights reserved. This is the accepted manuscript vers...
Unevolved metal poor stars are the witness of the early evolution of the Galaxy. The determination o...
6We present detailed chemical element abundance ratios of 17 elements with eight ≤ Z ≤ 60 in three...
Metal-poor stars provide information on the characteristics and chemical evolution of the halo popul...
Abstract The characteristics of the stellar populations in the Galactic Bulge inform and constrain t...
We present high-resolution Magellan/MIKE spectroscopy of the brightest star in the ultra-faint dwarf...
We present a high spectral resolution survey of the most metal-poor damped Lyα absorption systems (D...
Metal-poor stars in the Milky Way are local relics of the epoch of the first stars and the first gal...
Early-type dwarfs (ETDs) are the end points of the evolution of low-mass galaxies whose gas supply h...
We present new Keck/HIRES data of the most metal-poor damped Lyman-alpha (DLA) system currently know...
We report a method of identifying candidate low-metallicity blue compact dwarf galaxies (BCDs) from ...
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 report two new low-metallicity blue compact dwarf galaxies (BCDs), WISEP J080103.93+264053.9 (her...
In this paper we analyze the kinematics, chemistry, and physical properties of a sample of the most ...
© 2021. The American Astronomical Society. All rights reserved. This is the accepted manuscript vers...
Unevolved metal poor stars are the witness of the early evolution of the Galaxy. The determination o...
6We present detailed chemical element abundance ratios of 17 elements with eight ≤ Z ≤ 60 in three...
Metal-poor stars provide information on the characteristics and chemical evolution of the halo popul...
Abstract The characteristics of the stellar populations in the Galactic Bulge inform and constrain t...
We present high-resolution Magellan/MIKE spectroscopy of the brightest star in the ultra-faint dwarf...
We present a high spectral resolution survey of the most metal-poor damped Lyα absorption systems (D...
Metal-poor stars in the Milky Way are local relics of the epoch of the first stars and the first gal...
Early-type dwarfs (ETDs) are the end points of the evolution of low-mass galaxies whose gas supply h...
We present new Keck/HIRES data of the most metal-poor damped Lyman-alpha (DLA) system currently know...