Results 121 to 130 of about 692 (185)
Causal Discovery of Latent Variables in Galactic Archaeology
Accepted to ML4Astro 2025 (Machine Learning for Astrophysics workshop at ICML 2025)
Jin, Zehao +4 more
openaire +2 more sources
Stars in an open cluster are assumed to have formed from a broadly homogeneous distribution of gas, implying that they should be chemically homogeneous.
Amaya Sinha +6 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
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
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
The GALAH Survey and Galactic Archaeology in the next decade
The field of Galactic Archaeology aims to understand the origins and evolution of the stellar populations in the Milky Way, as a way to understand galaxy formation and evolution in general. The GALAH (Galactic Archaeology with HERMES) Survey is an ambitious Australian-led project to explore the Galactic history of star formation, chemical evolution ...
openaire +2 more sources
Galactic archaeology and its application to the galactic center
L'archéologie galactique consiste à disséquer et analyser les nombreuses composantes de la Voie Lactée afin de mettre en évidence et distinguer les processus physiques qui contribuent à sa formation et son évolution.
Nandakumar, Govind
core
Where are the most ancient stars in the Milky Way? [PDF]
El-Badry K +9 more
europepmc +1 more source
A direct black-hole mass measurement in a little red dot at high redshift. [PDF]
Juodžbalis I +39 more
europepmc +1 more source
Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars. [PDF]
Sun T +12 more
europepmc +1 more source

