Chemical gradients in the Milky Way from the RAVE data: I. Dwarf stars

Aims. We aim at measuring the chemical gradients of the elements Mg, Al, Si, and Fe along the Galactic radius to provide new constraints on the chemical evolution models of the Galaxy and Galaxy models such as the Besançon model. Thanks to the large number of stars of our RAVE sample we can study h...

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Main Authors: Boeche, Corrado (Author) , Siebert, A. (Author) , Piffl, T. (Author) , Just, Andreas (Author) , Steinmetz, M. (Author) , Sharma, S. (Author) , Kordopatis, G. (Author) , Gilmore, G. (Author) , Chiappini, C. (Author) , Williams, M. (Author) , Grebel, Eva K. (Author)
Format: Article (Journal)
Language:English
Published: 14 November 2013
In: Astronomy and astrophysics
Year: 2013, Volume: 559, Pages: 1-12
ISSN:1432-0746
DOI:10.1051/0004-6361/201322085
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/201322085
Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2013/11/aa22085-13/aa22085-13.html
Resolving-System, kostenfrei, Volltext: http://www.aanda.org/articles/aa/abs/2013/11/aa22085-13/aa22085-13.html
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Author Notes:C. Boeche, A. Siebert, T. Piffl, A. Just, M. Steinmetz, S. Sharma, G. Kordopatis, G. Gilmore, C. Chiappini, M. Williams, E.K. Grebel, J. Bland-Hawthorn, B.K. Gibson, U. Munari, A. Siviero, O. Bienaymé, J.F. Navarro, Q.A. Parker, W. Reid, G.M. Seabroke, F.G. Watson, R.F.G. Wyse, and T. Zwitter
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Chemical gradients in the Milky Way from the RAVE data: I. Dwarf stars


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