- Abstract:
-
We present evidence from the RAdial Velocity Experiment (RAVE) survey of chemically separated, kinematically distinct disc components in the solar neighbourhood.We apply probabilistic chemical selection criteria to separate our sample into α-low (‘thin disc’) and α-high (‘thick disc’) sequences. Using newly derived distances,which will be utilized in the upcoming RAVE DR5, we explore the kinematic trends as a function of metallicity for each of the disc components. For our α-low disc, we find...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 1.1MB)
-
- Publisher copy:
- 10.1093/mnras/stw1633
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 461
- Issue:
- 4
- Pages:
- 4246-4255
- Publication date:
- 2016-07-05
- Acceptance date:
- 2016-07-05
- DOI:
- EISSN:
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1365-2966
- ISSN:
-
0035-8711
- Pubs id:
-
pubs:742099
- URN:
-
uri:ae10622c-af79-4389-b536-8156330a99a9
- UUID:
-
uuid:ae10622c-af79-4389-b536-8156330a99a9
- Local pid:
- pubs:742099
- Copyright holder:
- Binney et al
- Copyright date:
- 2016
- Notes:
- © 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal article
Chemical separation of disc components using RAVE
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Australian Astronomical Observatory
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Leibniz-Institut fuer Astrophysik Potsdam
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Australian National University
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Australian Research Counci
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French National Research Agency
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