Results 141 to 150 of about 329,644 (212)
An archaeological evaluation was undertaken by Cotswold Archaeology in December 2015 at Walton Manor, Brickhill Street, Milton Keynes. The fieldwork was undertaken to inform a planning application to Milton Keynes Council for the construction of a ...
Cotswold Archaeology
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Land Warfare Centre, Warminster (OASIS id: wessexar1-92170)
Wessex Archaeology was commissioned by Aspire Defence Capital Works (the Client) to undertake an archaeological watching brief during groundworks at WXC605, WT0609 and WT0610, Land Warfare Centre, Warminster, Wiltshire, centred on National Grid Reference
Wessex Archaeology
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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
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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
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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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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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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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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Stellar streams for Galactic and cosmic archaeology
Les courants stellaires pour l'archéologie galactique et cosmique La mission astrométrique Gaia a permis l'étude à grande échelle des étoiles et des sous-structures galactiques. Environ 160 amas globulaires (AG) de la Voie lactée, chacun contenant de centaines de milliers à plusieurs millions d'étoiles, peuvent désormais être ...
openaire +2 more sources
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

