Improved oscillator strengths and wavelengths for Os I and Ir I, and new results on earlyr-process nucleosynthesis-Reference-Cited by-同舟云学术

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Improved oscillator strengths and wavelengths for Os I and Ir I, and new results on earlyr-process nucleosynthesis

Published:2003-10 Issue:3 Volume:409 Page:1141-1149
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Ivarsson S.,Andersen J.,Nordström B.,Dai X.,Johansson S.,Lundberg H.,Nilsson H.,Hill V.,Lundqvist M.,Wyart J. F.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20031184/pdf

Reference25 articles.

1. Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

2. Measurement of stellar age from uranium decay

3. Corliss, C. H., & Bozman, W. R. 1962, NBS Monograph, 53

4. The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248

5. Cowan, R. D. 1981, The Theory of Atomic Structure and Spectra (Berkley: Univ. of California Press)

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