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Chemodynamical modelling of the Milky Way

Abstract:
Chemodynamical models of our Galaxy that have analytic Extended Distribution Functions (EDFs) are likely to play a key role in extracting science from surveys in the era of Gaia.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1002/asna.201612403

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Oxford college:
Merton College
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Theoretical Physics
Role:
Author
Publisher:
Wiley Publisher's website
Journal:
Astronomische Nachrichten Journal website
Volume:
337
Issue:
8-9
Pages:
939-943
Publication date:
2016-09-30
Acceptance date:
2016-06-13
DOI:
EISSN:
0004-6337
ISSN:
1521-3994
Source identifiers:
797941
Keywords:
Pubs id:
pubs:797941
UUID:
uuid:6674bff1-5c0f-4f44-9675-de29ab916285
Local pid:
pubs:797941
Deposit date:
2018-01-23

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