The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling-Reference-Cited by-同舟云学术

The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling

Published:2020-05-18 Issue:4 Volume:216 Page:
ISSN:0038-6308
Container-title:Space Science Reviews
language:en
Short-container-title:Space Sci Rev

Author:

Cavalié Thibault^ORCID,Venot Olivia,Miguel Yamila,Fletcher Leigh N.,Wurz Peter,Mousis Olivier,Bounaceur Roda,Hue Vincent,Leconte Jérémy,Dobrijevic Michel

Funder

Programme National de Planétologie

CNES

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://link.springer.com/content/pdf/10.1007/s11214-020-00677-8.pdf

Reference245 articles.

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3. A.M. Amarsi, M. Asplund, The solar silicon abundance based on 3D non-LTE calculations. Mon. Not. R. Astron. Soc. 464(1), 264–273 (2017). https://doi.org/10.1093/mnras/stw2445

4. A.M. Amarsi, P.S. Barklem, M. Asplund, R. Collet, O. Zatsarinny, Inelastic O+H collisions and the O I 777 nm solar centre-to-limb variation. Astron. Astrophys. 616, A89 (2018). https://doi.org/10.1051/0004-6361/201832770

5. A.M. Amarsi, P.S. Barklem, R. Collet, N. Grevesse, M. Asplund, 3D non-LTE line formation of neutral carbon in the Sun. Astron. Astrophys. 624, A111 (2019). https://doi.org/10.1051/0004-6361/201833603

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