Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars-Reference-Cited by-同舟云学术

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Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars

Published:2010-10 Issue: Volume:521 Page:L57
ISSN:0004-6361
Container-title:Astronomy and Astrophysics
language:
Short-container-title:A&A

Author:

Bensby T.,Asplund M.,Johnson J. A.,Feltzing S.,Meléndez J.,Dong S.,Gould A.,Han C.,Adén D.,Lucatello S.,Gal-Yam A.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201015745/pdf

Reference44 articles.

2. LITHIUM ABUNDANCES OF EXTREMELY METAL-POOR TURNOFF STARS

3. Multi-level 3D non-LTE computations of lithium lines in the metal-poor halo stars HD 140283 and HD 84937

4. Lithium Isotopic Abundances in Metal‐poor Halo Stars

5. The Chemical Composition of the Sun

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1. Sulfur abundances in the Galactic bulge and disk;Astronomy & Astrophysics;2021-12-22

2. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars;Astronomy & Astrophysics;2020-02

3. De re metallica: the cosmic chemical evolution of galaxies;The Astronomy and Astrophysics Review;2019-02-04

4. Chemical Evolution of the Milky Way and Its Satellites;The Origin of the Galaxy and Local Group;2014

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