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:2009-04-08 Issue:3 Volume:499 Page:737-753
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Bensby T.,Johnson J. A.,Cohen J.,Feltzing S.,Udalski A.,Gould A.,Huang W.,Thompson I.,Simmerer J.,Adén D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/200911629/pdf

Reference73 articles.

1. Width cross-sections for collisional broadening of s–p and p–s transitions by atomic hydrogen

2. New Light on Stellar Abundance Analyses: Departures from LTE and Homogeneity

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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;2021-11

3. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars;Astronomy & Astrophysics;2017-09

4. The age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way;Proceedings of the International Astronomical Union;2017-07

5. The Galaxy in Context: Structural, Kinematic, and Integrated Properties;Annual Review of Astronomy and Astrophysics;2016-09-19

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