Lachlan Lancaster
The Halo’s Ancient Metal-Rich Progenitor Revealed with BHB Stars
Lancaster, Lachlan; Koposov, Sergey E; Belokurov, Vasily; Evans, N Wyn; Deason, Alis J
Authors
Sergey E Koposov
Vasily Belokurov
N Wyn Evans
Professor Alis Deason alis.j.deason@durham.ac.uk
Professor
Abstract
Using the data from the Sloan Digital Sky Survey and the Gaia satellite, we assemble a pure sample of ∼3000 Blue Horizontal Branch (BHB) stars with 7-D information, including positions, velocities and metallicities. We demonstrate that, as traced with BHBs, the Milky Way’s stellar halo is largely unmixed and can not be well represented with a conventional Gaussian velocity distribution. A single-component model fails because the inner portions of the halo are swamped with metal-rich tidal debris from an ancient, head-on collision, known as the “Gaia Sausage”. Motivated by the data, we build a flexible mixture model which allows us to track the evolution of the halo make-up across a wide range of radii. It is built from two components, one representing the radially anisotropic Sausage stars with their lobed velocity distribution, the other representing a more metal-poor and more isotropic component built up from minor mergers. We show that inside 25 kpc the “Sausage” contributes at least 50% of the Galactic halo. The fraction of “Sausage” stars diminishes sharply beyond 30 kpc, which is the long-established break radius of the classical stellar halo.
Citation
Lancaster, L., Koposov, S. E., Belokurov, V., Evans, N. W., & Deason, A. J. (2019). The Halo’s Ancient Metal-Rich Progenitor Revealed with BHB Stars. Monthly Notices of the Royal Astronomical Society, 486(1), 378-389. https://doi.org/10.1093/mnras/stz853
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 18, 2019 |
Online Publication Date | Mar 27, 2019 |
Publication Date | Jun 30, 2019 |
Deposit Date | Apr 4, 2019 |
Publicly Available Date | Apr 11, 2019 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 486 |
Issue | 1 |
Pages | 378-389 |
DOI | https://doi.org/10.1093/mnras/stz853 |
Public URL | https://durham-repository.worktribe.com/output/1304543 |
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Copyright Statement
© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
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