Schiavon, RP, Mackereth, JT, Pfeffer, JL, Crain, RA and Bovy, J (2020) The building blocks of the Milky Way halo using APOGEE and Gaia -- or -- Is the Galaxy a typical galaxy? Proceedings of the International Astronomical Union, 14 (S351). pp. 170-173. ISSN 1743-9213
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Abstract
We summarise recent results from analysis of APOGEE/Gaia data for stellar populations in the Galactic halo, disk, and bulge, leading to constraints on the contribution of dwarf galaxies and globular clusters to the stellar content of the Milky Way halo. Interpretation of the extant data in light of cosmological numerical simulations suggests that the Milky Way has been subject to an unusually intense accretion history at z >~ 1.5.
Item Type: | Article |
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Uncontrolled Keywords: | 0201 Astronomical and Space Sciences |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Divisions: | Astrophysics Research Institute |
Publisher: | Cambridge University Press |
Related URLs: | |
Date Deposited: | 20 Apr 2021 11:25 |
Last Modified: | 04 Sep 2021 05:34 |
DOI or ID number: | 10.1017/S1743921319007889 |
URI: | https://researchonline.ljmu.ac.uk/id/eprint/14831 |
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