An overall picture of EMP stars using the stellar abundances for galactic archaeology (SAGA) database [PDF]
Takuma Suda +7 more
openalex +1 more source
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
doaj +1 more source
A time-resolved picture of our Milky Way's early formation history. [PDF]
Xiang M, Rix HW.
europepmc +1 more source
Galactic archaeology Using chemical abundances to map our galaxy’s history [PDF]
openalex +1 more source
Galactic Archaeology: Tracing the Milky Way's Formation and Evolution through Stellar Populations [PDF]
J. Alfredo Collazos
openalex +2 more sources
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
doaj +1 more source
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
Predicting the geographic distribution of ancient Amazonian archaeological sites with machine learning. [PDF]
Walker RS +5 more
europepmc +1 more source
THE K2 GALACTIC ARCHAEOLOGY PROGRAM DATA RELEASE I: ASTEROSEISMIC RESULTS FROM CAMPAIGN 1 [PDF]
Dennis Stello +13 more
openalex +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
doaj +1 more source

