THE K2 GALACTIC ARCHAEOLOGY PROGRAM DATA RELEASE I: ASTEROSEISMIC RESULTS FROM CAMPAIGN 1 [PDF]
Dennis Stello +13 more
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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 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
Galactic archaeology Using chemical abundances to map our galaxy’s history [PDF]
openalex +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
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Galactic Archaeology: Tracing the Milky Way's Formation and Evolution through Stellar Populations [PDF]
J. Alfredo Collazos
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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
doaj +1 more source
Galactic archaeology for amateur astronomers: RR Lyrae stars as tracers of the Milky Way formation [PDF]
J. A. Carballo-Bello +2 more
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Prospects for IXPE and eXTP polarimetric archaeology of the reflection nebulae in the Galactic center [PDF]
L. Di Gesu +7 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
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