Journal article
Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s)
- Abstract:
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Investigations of the origin and evolution of the Milky Way disc have long relied on chemical and kinematic identifications of its components to reconstruct our Galactic past. Difficulties in determining precise stellar ages have restricted most studies to small samples, normally confined to the solar neighbourhood. Here, we break this impasse with the help of asteroseismic inference and perform a chronology of the evolution of the disc throughout the age of the Galaxy. We chemically dissect ...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 2.8MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/sty150
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Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 475
- Issue:
- 4
- Pages:
- 5487–5500
- Publication date:
- 2018-01-18
- Acceptance date:
- 2018-01-15
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Keywords:
- Pubs id:
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pubs:844098
- UUID:
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uuid:8240ebb1-edbc-4a4b-9664-fe1b3d58982d
- Local pid:
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pubs:844098
- Source identifiers:
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844098
- Deposit date:
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2018-06-12
Terms of use
- Copyright holder:
- © 2018 Aguirre, et al Published by Oxford University Press on behalf of the Royal Astronomical Society
- Copyright date:
- 2018
- Notes:
- This is the publisher's version of the article. The final version is available online from Oxford University Press at: 10.1093/mnras/sty150. For the full funder list see the article
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