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The chemical characterisation of halo substructure in the Milky Way based on APOGEE

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The chemical characterisation of halo substructure in the Milky Way based on APOGEE

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2649432827

The chemical characterisation of halo substructure in the Milky Way based on APOGEE

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Ithaca: Cornell University Library, arXiv.org

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Contents

Galactic haloes in a \(\Lambda\)-CDM universe are predicted to host today a swarm of debris resulting from cannibalised dwarf galaxies. The chemo-dynamical information recorded in their stellar populations helps elucidate their nature, constraining the assembly history of the Galaxy. Using data from APOGEE and \textit{Gaia}, we examine the chemical...

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The chemical characterisation of halo substructure in the Milky Way based on APOGEE

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TN_cdi_proquest_journals_2649432827

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2649432827

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E-ISSN

2331-8422

DOI

10.48550/arxiv.2204.04233

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