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Chemical gradients in the Milky Way from the RAVE data. II. Giant stars

Abstract:

We provide new constraints on the chemo-dynamical models of the Milky Way by measuring the radial and vertical chemical gradients for the elements Mg, Al, Si, Ti, and Fe in the Galactic disc and the gradient variations as a function of the distance from the Galactic plane ($Z$). We selected a sample of giant stars from the RAVE database using the gravity criterium 1.7$<$log g$<$2.8. We created a RAVE mock sample with the Galaxia code based on the Besan\c con model and selected a corresp...

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Publisher copy:
10.1051/0004-6361/201423974

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author
Publisher:
EDP Sciences Publisher's website
Journal:
A
Volume:
568
Pages:
A71
Publication date:
2014-06-27
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Language:
English
Keywords:
Pubs id:
pubs:472173
UUID:
uuid:24dfdac7-9652-4c43-9f33-ea9a26cd4a18
Local pid:
pubs:472173
Source identifiers:
472173
Deposit date:
2014-07-19

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