A Swing of the Pendulum: The Chemodynamics of the Local Stellar Halo Indicate Contributions from Several Radial Merger Events

Abstract We find that the chemical abundances and dynamics of APOGEE and GALAH stars in the local stellar halo are inconsistent with a scenario in which the inner halo is primarily composed of debris from a single massive, ancient merger event, as has been proposed to explain the Gaia-Enceladus/Gaia...

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Bibliographic Details
Published in:The Astrophysical journal 2023-02, Vol.944 (2), p.169
Main Authors: Donlon, Thomas, Newberg, Heidi Jo
Format: Article
Language:English
Subjects:
Abundance
Accretion
Algorithms
Apogees
Astronomy & Astrophysics
Astrophysics
Chemical composition
Chemical evolution
Deposition
Enceladus
Galactic archaeology
Gaussian mixture model
Milky Way stellar halo
Mixtures
Probabilistic models
Regression models
Stars
Stellar astronomy
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Summary:Abstract We find that the chemical abundances and dynamics of APOGEE and GALAH stars in the local stellar halo are inconsistent with a scenario in which the inner halo is primarily composed of debris from a single massive, ancient merger event, as has been proposed to explain the Gaia-Enceladus/Gaia Sausage (GSE) structure. The data contain trends of chemical composition with energy that are opposite to expectations for a single massive, ancient merger event, and multiple chemical evolution paths with distinct dynamics are present. We use a Bayesian Gaussian mixture model regression algorithm to characterize the local stellar halo, and find that the data are fit best by a model with four components. We interpret these components as the Virgo Radial Merger (VRM), Cronus, Nereus, and Thamnos; however, Nereus and Thamnos likely represent more than one accretion event because the chemical abundance distributions of their member stars contain many peaks. Although the Cronus and Thamnos components have different dynamics, their chemical abundances suggest they may be related. We show that the distinct low- and high- α halo populations from Nissen & Schuster are explained by VRM and Cronus stars, as well as some in situ stars. Because the local stellar halo contains multiple substructures, different popular methods of selecting GSE stars will actually select different mixtures of these substructures, which may change the apparent chemodynamic properties of the selected stars. We also find that the Splash stars in the Solar region are shifted to higher v ϕ and slightly lower [Fe/H] than previously reported.
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/acb150