IMPROVING THE Ni I ATOMIC MODEL FOR SOLAR AND STELLAR ATMOSPHERIC MODELS

Author:

Vieytes M. C.,Fontenla J. M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 13 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. The Pristine survey – XXII. A serendipitous discovery of an extremely Li-rich very metal-poor giant and a new method of 6Li/7Li isotope measurement;Monthly Notices of the Royal Astronomical Society;2023-10-13

2. Detailed abundances of the wide pairs of stars with and without planets: the binary systems 16 Cyg and HD 219542;Monthly Notices of the Royal Astronomical Society;2022-06-20

3. Inelastic Processes in Nickel–Hydrogen Collisions;The Astrophysical Journal;2022-02-01

4. Modeling the Mg I from the NUV to MIR;Astronomy & Astrophysics;2022-01

5. Solar oxygen abundance;Monthly Notices of the Royal Astronomical Society;2021-07-30

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