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: | , , , , , , , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
14 November 2013
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| 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 |
| 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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