A unique hot Jupiter spectral sequence with evidence for compositional diversity-Reference-Cited by-同舟云学术

A unique hot Jupiter spectral sequence with evidence for compositional diversity

Published:2021-10-21 Issue:12 Volume:5 Page:1224-1232
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Mansfield Megan^ORCID,Line Michael R.^ORCID,Bean Jacob L.,Fortney Jonathan J.,Parmentier Vivien,Wiser Lindsey^ORCID,Kempton Eliza M.-R.^ORCID,Gharib-Nezhad Ehsan,Sing David K.^ORCID,López-Morales Mercedes,Baxter Claire,Désert Jean-Michel,Swain Mark R.,Roudier Gael M.^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01455-4.pdf

Reference77 articles.

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3. Parmentier, V. et al. From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context. Astron. Astrophys. 617, A110 (2018).

4. Arcangeli, J. et al. H− opacity and water dissociation in the dayside atmosphere of the very hot gas giant WASP-18b. Astrophys. J. Lett. 855, L30 (2018).

5. Kreidberg, L. et al. A precise water abundance measurement for the hot Jupiter WASP-43b. Astrophys. J. Lett. 793, L27 (2014).

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