The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
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Author / Creator
Horta, Danny , Mackereth, J Ted , Schiavon, Ricardo P , Hasselquist, Sten , Bovy, Jo , Carlos Allende Prieto , Beers, Timothy C , Cunha, Katia , García-Hernández, D A , Kisku, Shobhit S , Lane, Richard R , Majewski, Steven R , Mason, Andrew C , Nataf, David M , Roman-Lopes, Alexandre and Schultheis, Mathias
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
The contribution of dissolved globular clusters (GCs) to the stellar content of the Galactic halo is a key constraint on models for GC formation and destruction, and the mass assembly history of the Milky Way. Earlier results from APOGEE pointed to a large contribution of destroyed GCs to the stellar content of the inner halo, by as much as 25\(\%\...
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Full title
The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
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Record Identifier
TN_cdi_proquest_journals_2430536692
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2430536692
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.2008.01097
