Results 101 to 110 of about 5,324 (165)

Chemical Abundances in the Nuclear Star Cluster of the Milky Way: Alpha-element Trends and Their Similarities with the Inner Bulge

open access: yesThe Astrophysical Journal
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

open access: yesThe Astronomical Journal
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

Potassium Abundances in Extremely Metal Poor Stars: Implications for Nucleosynthesis in the Final Stages of Massive Star Evolution

open access: yesThe Astrophysical Journal
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]

open access: bronze, 2014
L. Casagrande   +19 more
openalex   +1 more source

Watching Our Galaxy Grow Up: The Mass and Color Evolution of the Milky Way

open access: yesThe Astrophysical Journal
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

open access: yes, 2012
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  

MEASNet. I. A Model for Barium Star Identification and s-process Abundance Estimation from LAMOST DR10 Low-resolution Survey

open access: yesThe Astrophysical Journal
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]

open access: bronze, 2015
S. Comerón   +4 more
openalex   +1 more source

Stellar archaeology with Gaia: the Galactic white dwarf population

open access: yes, 2015
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)

open access: diamond, 2023
Mario Ortigoza-Urdaneta   +9 more
openalex   +1 more source

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