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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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Date

2010

Authors

Bensby, T
Asplund, Martin
Johnson, Jennifer A
Feltzing, Sofia
Melendez, Jorge
Dong, S
Gould, A
Han, C
Aden, Daniel
Lucatello, Sara

Journal Title

Journal ISSN

Volume Title

Publisher

Springer

Abstract

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

Description

Keywords

Keywords: Chemical compositions; Chemical evolution; Dwarf stars; Elemental abundance; Galactic bulge; Galactic disks; Galaxy: bulge; Galaxy: formation - Galaxy: evolution; Gravitational lensing; High resolution; Line profiles; Metallicities; Micro-lensing; Old age Galaxy: bulge; Galaxy: formation - Galaxy: evolution; gravitational lensing: micro; stars: abundances

Citation

URI

http://hdl.handle.net/1885/79518

Collections

ANU Research Publications

Source

Astronomy and Astrophysics

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1051/0004-6361/201015745

Restricted until

2037-12-31

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