Chronologically dating the early assembly of the Milky Way
Josefina Montalb\'an (1), John Ted Mackereth (1,2,3, 4), Andrea, Miglio (1,5, 6), Fiorenzo Vincenzo (1,7, 8), Cristina Chiappini (9),, Ga\"el Buldgen (10), Beno\^it Mosser (11), Arlette Noels (12), Richard, Scuflaire (12), Mathieu Vrard (8, 13), Emma Willett (1, 14), Guy R.

TL;DR
This study combines asteroseismology, kinematics, and chemical data to precisely date stars in the Milky Way, revealing that significant stellar populations existed before the major Gaia-Enceladus/Sausage merger around 10 billion years ago.
Contribution
It introduces a method integrating stellar oscillations with kinematic and chemical data to accurately date ancient stars, including those accreted from external galaxies.
Findings
The Milky Way had a substantial stellar population before the Gaia-Enceladus/Sausage merger.
Stars formed both inside and outside the Galaxy can be precisely aged using this method.
The Galaxy's thick disc contains stars formed prior to the major merger event.
Abstract
The standard cosmological model (-CDM) predicts that galaxies are built through hierarchical assembly on cosmological timescales. The Milky Way, like other disc galaxies, underwent violent mergers and accretion of small satellite galaxies in its early history. Thanks to Gaia-DR2 and spectroscopic surveys, the stellar remnants of such mergers have been identified. The chronological dating of such events is crucial to uncover the formation and evolution of the Galaxy at high redshift, but it has so far been challenging owing to difficulties in obtaining precise ages for these oldest stars. Here we combine asteroseismology -- the study of stellar oscillations -- with kinematics and chemical abundances, to estimate precise stellar ages ( 11%) for a sample of stars observed by the space mission. Crucially, this sample includes not…
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