Milky Way's Eccentric Constituents with Gaia, APOGEE, and GALAH [PDF]
We report the results of an unsupervised decomposition of the local stellar halo in the chemodynamical space spanned by the abundance measurements from APOGEE DR17 and GALAH DR3.
G. Myeong+11 more
semanticscholar +1 more source
Can Neutron Star Mergers Alone Explain the r-process Enrichment of the Milky Way? [PDF]
Comparing Galactic chemical evolution models to the observed elemental abundances in the Milky Way, we show that neutron star mergers can be a leading r-process site only if at low metallicities such mergers have very short delay times and significant ...
C. Kobayashi+11 more
semanticscholar +1 more source
Chemical evolution of the Milky Way: the origin of phosphorus [PDF]
Context. Recently, for the first time the abundance of P has been measured in disk stars. This provides the opportunity of comparing the observed abundances with predictions from theoretical models. Aims. We aim at predicting the chemical evolution of P in the Milky Way and compare our results with the observed P abundances in disk stars in order to ...
P. Francois+6 more
openaire +6 more sources
ATLAS probe: Breakthrough science of galaxy evolution, cosmology, Milky Way, and the Solar System [PDF]
Astrophysics Telescope for Large Area Spectroscopy Probe is a concept for a National Aeronautics and Space Administration probe-class space mission that will achieve ground-breaking science in the fields of galaxy evolution, cosmology, Milky Way, and the
Yun Wang+47 more
semanticscholar +1 more source
Stellar Bars in Isolated Gas-rich Spiral Galaxies Do Not Slow Down
Elongated bar-like features are ubiquitous in galaxies, occurring at the centers of approximately two-thirds of spiral disks in the nearby Universe. Due to gravitational interactions between the bar and the other components of galaxies, it is expected ...
Angus Beane+8 more
doaj +1 more source
Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution
Stellar ages are key for determining the formation history of the Milky Way, but are difficult to measure precisely. Furthermore, methods that use chemical abundances to infer ages may entangle the intrinsic evolution of stars with the chemodynamical ...
Jeff Shen+4 more
doaj +1 more source
The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream [PDF]
It has recently been shown that the Large Magellanic Cloud (LMC) has a substantial effect on the Milky Way’s stellar halo and stellar streams. Here, we explore how deformations of the Milky Way and LMC’s dark matter haloes affect stellar streams, and ...
Sophia Lilleengen+15 more
semanticscholar +1 more source
Widespread Detection of Two Components in the Hot Circumgalactic Medium of the Milky Way [PDF]
Surrounding the Milky Way (MW) is the circumgalactic medium (CGM), an extended reservoir of hot gas that has significant implications for the evolution of the MW.
J. Bluem+8 more
semanticscholar +1 more source
The AMBRE Project: Origin and evolution of sulfur in the Milky Way [PDF]
Context. Sulfur is a volatile chemical element that plays an important role in tracing the chemical evolution of the Milky Way and external galaxies. However, its nucleosynthesis origin and abundance variations in the Galaxy are still unclear because the number of available stellar sulfur abundance measurements is currently rather small. Aims. The goal
Perdigon, J.+6 more
openaire +5 more sources
The Formalism of Milky-Way Antimatter-Domains Evolution
If baryosynthesis is strongly nonhomogeneous, macroscopic regions with antibaryon excess can be created in the same process from which the baryonic matter is originated. This exotic possibility can become real, if the hints to the existence of antihelium
Maxim Yu. Khlopov, Orchidea Maria Lecian
doaj +1 more source