- Abstract:
-
Aim: 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 Besancon model. Methods: We analysed three different samples selected from three independent datasets: a sample of 19,962 dwarf stars selected from the RAVE database, a sample of 10,616 dwarf stars selected from the Geneva-Copenhagen Survey (GCS) dataset, and a mock sample (equival...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1051/0004-6361001423974
-
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- Journal:
- ASTRONOMY and ASTROPHYSICS
- Volume:
- 568
- Pages:
- A59-A59
- Publication date:
- 2013-09-17
- DOI:
- EISSN:
-
1432-0746
- ISSN:
-
0004-6361
- URN:
-
uuid:78e9d4cb-f6a4-4590-a290-fe5f40b8ff48
- Source identifiers:
-
441336
- Local pid:
- pubs:441336
- Language:
- English
- Keywords:
- Copyright date:
- 2013
- Notes:
- Accepted for publication in AandA
Journal article
Chemical gradients in the Milky Way from the RAVE data. I. Dwarf stars
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