Interpretation of Ti I lines of excitation energy 0.0-0.05 eV in the solar spectrum; use of new oscillator strengths of accuracy 0.5 per cent-Reference-Cited by-同舟云学术

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Interpretation of Ti I lines of excitation energy 0.0-0.05 eV in the solar spectrum; use of new oscillator strengths of accuracy 0.5 per cent

Published:1982-05-01 Issue:1 Volume:199 Page:37-42
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Blackwell D. E.,Shallis M. J.,Simmons G. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/199/1/37/4167793/mnras199-0037.pdf

Cited by 12 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Photometric and polarimetric clues to the circumstellar environment of RY Lupi;Astronomy & Astrophysics;2009-03-25

2. Abundances of the heavy elements in the Magellanic Clouds. III - Interpretation of results;The Astrophysical Journal;1992-01

3. Relative abundance determinations in extremely metal poor giants. II - Transition probabilities and the abundance determinations;The Astrophysical Journal;1990-02

4. Abundances of the heavy elements in the Magellanic Clouds. I - Metal abundances of F-type supergiants;The Astrophysical Journal Supplement Series;1989-08

5. The measurement of oscillator strengths;Reports on Progress in Physics;1986-04-01

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