Asteroseismology of Metal-poor Red Giants Observed by TESS
Galactic archeology has long been limited by a lack of precise masses and ages for metal-poor stars in the Milky Way’s thick disk. However, with TESS providing a growing number of photometric observations, it is possible to calculate masses and ages for ...
Corin Marasco +2 more
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A Wave-corrected Assessment of the Local Midplane
As the number of known Galactic structures mounts thanks to the Gaia Space Telescope, it is now pertinent to study methods for disentangling structures occupying the same regions of the Milky Way. Indeed, understanding the precise form of each individual
Ziyuan Yin, Austin Hinkel
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The Stellar Abundances for Galactic Archaeology (SAGA) Database – III. Analysis of enrichment histories for elements and two modes of star formation during the early evolution of the Milky Way [PDF]
Shimako Yamada +4 more
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On the Origin of Neutron-capture Elements in r-I and r-II Stars: A Differential-abundance Analysis
We present a strictly line-by-line differential analysis of a moderately r -process-enhanced star ( r -I: HD 107752) with respect to a strongly r -process-enhanced star ( r -II: CS 31082-0001) to investigate the possible common origin of their heavy ...
Pallavi Saraf +6 more
doaj +1 more source
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
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Galactic Archaeology with asteroseismic ages: Evidence for delayed gas infall in the formation of the Milky Way disc [PDF]
E. Spitoni +4 more
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The R-process Alliance: Enrichment of r-process Elements in a Simulated Milky Way–like Galaxy
We study the formation of stars with varying amounts of heavy elements synthesized by the rapid neutron-capture process ( r -process) based on our detailed cosmological zoom-in simulation of a Milky Way–like galaxy with an N -body/smoothed particle ...
Yutaka Hirai +13 more
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Detection of early-universe gravitational-wave signatures and fundamental physics. [PDF]
Caldwell R +37 more
europepmc +1 more source
Galactic archaeology with the oldest stars in the Milky Way
Anke Arentsen
openalex +2 more sources
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
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