Proof that the Milky Way experienced a significant merger only 1.5 billion years after the Big Bang
Davide Massari, Chiara Zerbinati, Cristiano Fanelli, Amina Helmi, Edoardo Ceccarelli, Fernando Aguado-Agelet, Santi Cassisi, Ewoud Wempe, Matteo Monelli, Andrea Bellini, Thomas Callingham, Hanneke C. Woudenberg, Roger Cohen, Carme Gallart, Elena Pancino, Sara Saracino

TL;DR
This study reveals that the Milky Way experienced a significant merger only 1.5 billion years after the Big Bang, based on detailed analysis of globular cluster populations using Hubble data.
Contribution
It provides the first direct evidence of a major merger in the early history of the Milky Way, identifying a new progenitor system called LKH.
Findings
Identified three distinct globular cluster age-metallicity sequences.
Discovered a merger event 1.5 billion years after the Big Bang.
Estimated the progenitor's stellar mass at ~5x10^8 solar masses.
Abstract
The merger history of the Galaxy has been traced back firmly to redshift 2 (10 Billion years ago). While there have been claims of the existence of at least one more significant merger before this time, supporting evidence has been indirect and contentious. Here we show that the population of globular clusters around the Galaxy depicts three distinct age-metallicity sequences, one associated with the merger with Gaia-Enceladus 10 billion years ago, one to the progenitor of the Milky Way and a third intermediate sequence associated to at least one merger which we estimate took place merely 1.5 billion years after the Big Bang. This discovery has been possible thanks to exquisite Hubble Space Telescope data and sophisticated analysis that enables very precise relative age determination of globular clusters. The newly identified sequence reveals that this merger took place with an object…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
