Implications ofWMAPObservations on Li Abundance and Stellar Evolution Models-Reference-Cited by-同舟云学术

Implications ofWMAPObservations on Li Abundance and Stellar Evolution Models

Published:2005-01-20 Issue:1 Volume:619 Page:538-548
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Richard O.,Michaud G.,Richer J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/619/i=1/a=538/pdf

Reference71 articles.

1. Diffusion in the Sun.

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

3. Balachandran, S. C. 2000, in IAU Symp. 198, The Light Elements and their Evolution, ed. L. Da Silva, M. Spite, R. de Medeiros (San Francisco: ASP), 383

4. Inelastic H+Li and H-+Li+collisions and non-LTE Li I line formation in stellar atmospheres

5. Angular Momentum Transport in Magnetized Stellar Radiative Zones. III. The Solar Light‐Element Abundances

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