Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S
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Bensby, T; Asplund, Martin; Johnson, Jennifer A; Feltzing, Sofia; Melendez, Jorge; Dong, S; Gould, A; Han, C; Aden, Daniel; Lucatello, Sara; Gal-Yam, Avishay
Description
Context. To study the evolution of Li in the Galaxy it is necessary to observe dwarf or subgiant stars. These are the only long-lived stars whose present-day atmospheric chemical composition reflects their natal Li abundances according to standard models
| Collections | ANU Research Publications |
|---|---|
| Date published: | 2010 |
| Type: | Journal article |
| URI: | http://hdl.handle.net/1885/79518 |
| Source: | Astronomy and Astrophysics |
| DOI: | 10.1051/0004-6361/201015745 |
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| File | Description | Size | Format | Image |
|---|---|---|---|---|
| 01_Bensby_Chemical_evolution_of_the_2010.pdf | 158.42 kB | Adobe PDF | Request a copy |
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