Results 101 to 110 of about 5,324 (165)
Chemical characterization of the Galactic center is essential for understanding its formation and structural evolution. Trends of alpha ( α ) elements, such as magnesium, silicon, and calcium, serve as powerful diagnostic tools, offering insights into ...
Nils Ryde +17 more
doaj +1 more source
UNIONS: The Ultraviolet Near-infrared Optical Northern Survey
The Ultraviolet Near-Infrared Optical Northern Survey (UNIONS) is a “collaboration of collaborations” that is using the Canada–France–Hawai’i Telescope, the Pan-STARRS telescopes, and the Subaru Observatory to obtain ugriz images of a core survey region ...
Stephen Gwyn +88 more
doaj +1 more source
We present a potassium (K) abundance analysis in extremely metal-poor (EMP) stars based on high-resolution ( R ∼ 60,000) spectra obtained with the High Dispersion Spectrograph on the Subaru Telescope, covering the K i resonance lines at 766 and 769 nm ...
Miho N. Ishigaki +8 more
doaj +1 more source
STRÖMGREN SURVEY FOR ASTEROSEISMOLOGY AND GALACTIC ARCHAEOLOGY: LET THE SAGA BEGIN [PDF]
L. Casagrande +19 more
openalex +1 more source
Watching Our Galaxy Grow Up: The Mass and Color Evolution of the Milky Way
Using our rich observations within the Milky Way to better understand galaxy evolution requires understanding what the Milky Way looks like “as a galaxy”—that is, its “true” shape and abundance profiles (unskewed by observational biases), signatures of ...
Gail Zasowski +2 more
doaj +1 more source
Chemical Evolution of the Carina Dwarf Spheroidal
We explore a range of chemical evolution models for the Local Group dwarf spheroidal (dSph) galaxy, Carina. A novel aspect of our work is the removal of the star formation history (SFH) as a `free parameter' in the modeling, making use, instead, of its ...
Gibson, B. K., Pilkington, K.
core
Barium stars are peculiar stars with enhanced slow neutron capture process ( s -process) elements. Abundance analysis of them aids in better understanding the chemical evolution of the Milky Way. In this paper, we introduce a data-driven method named the
Shengjun Song +4 more
doaj +1 more source
Galactic archaeology of a thick disc: Excavating ESO 533-4 with VIMOS [PDF]
S. Comerón +4 more
openalex +1 more source
Stellar archaeology with Gaia: the Galactic white dwarf population
Gaia will identify several 1e5 white dwarfs, most of which will be in the solar neighborhood at distances of a few hundred parsecs. Ground-based optical follow-up spectroscopy of this sample of stellar remnants is essential to unlock the enormous ...
Barcells, M. +26 more
core
Galactic ArchaeoLogIcaL ExcavatiOns (GALILEO)
Mario Ortigoza-Urdaneta +9 more
openalex +1 more source

